DOCSLIB.ORG

Prof.Dr. Şölen BALMAN

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Prof.Dr. Şölen BALMAN Prof.Dr. Şölen BALMAN İKşi Tşiesleflo Bniul:g +il9e0r 212 440 0000 Dahili: 10668-7 DE-ipğeors tEa-:p soosletna.:b saolmleann.b@[email protected] PWoesbta: hAtdtprse:/s/i:a vPersoifs. .iDstra. nSbouleln.e dBua.ltmr/a6n9 I2s1ta4nbul University Astronomy and Space Sciences Beyazit, 34119, Istanbul, Turkey EBüğtiütnimleş iBk iDlgokilteorai, University of Wisconsin-Madison, Colledge of Letters and Science, Physics, Amerika Birleşik LDiesvalnest,l eBroi ğ1a9z9iç2i -Ü 1n9iv9e7rsitesi, Fen-Edebiyat Fakültesi, Fizik Bölümü, Türkiye 1987 - 1991 Yİnagbiliazcnec, Cı 1D İilellreir SMeerslteikfi kEğai,t iKmu, Irnstr ovdeu cEtiğoint itmo SlPeArCE SYSTEMS ENGINEERING” course by Prof. Dr. S. Gabriel, School of Engineering DSciğieenrc, eFsin, Ae eArrotssp (aMcein Eonrg),i nBeoegrainzigc,i UUnniivv. eorfs Sitoyu, 1th9a8m7pton, European Space Agency, 2006 Yaptığı Tezler GBaültaücntilce şNiko vDaoek, tUonraiv, eXr-sRitayy oEfm Wisisicoonn sfrino-mM aCdlaisosinc,a Fl eNno-vEadee biniy Oaut tFbaukrüsltt:e Nsio, vFaiz Ciky, g1n9i9 17992 and Other ROSAT Detections of ATermaeşlt Bırilmimale rA, Mlaünhleanrdıislik ve Teknoloji Akademik Unvanlar / Görevler ÖYrğdre.Dtiomç .DGör.r, eOvrltiasi DDorğ., uO Trteak Dniokğ Üun Tiveekrnsiikt eÜsni, iFverns-iEtedseib, Fiyeant -FEadkeüblityeasti , FFaizkiükl tBeösil,ü Fmizüik, 1 B9ö9l9ü m- 2ü0, 109297 - 1999 ABAkPa Bdielimsiekl Kİodmairsiy oDne Ünyeeysii, mOrta Doğu Teknik Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, 2013 - 2018 FBaÖkLüÜltMe KBuArŞuKluA NÜ yDeAsiN, OIŞrMtaA DNoI,ğ Our Ttae kDnoikğ uÜ Tneivkenriski tÜensii,v Feernsi-tEedsie, bFieyna-tE Fdaekbüilytaets iF, aFkizüiklt eBsöi,l üFmiziük, B2ö0l0ü0m -ü 2, 020309 - 2012 SCI. I, STShCe IU vLeX AsoHuCrcIe İ nX-d3e ikns NleGrCi n4e2 5G8i:r ae nse Darecrhg ifloerr idtse XY-raayyı nalnadn oapnt iMcaal kparolepleerrties MAkOyNuTz HAL., YA NvdOaTnI CSE., SA OllaFk T SH.,E A RksOaYkAeLr NAS., TORrOalNhOanM II.C AA. L, BSaOlCmIEanT YŞ,. cilt.499, sa.2, ss.2138-2147, 2020 (SCI İndekslerine II. XG-irreany Dperrogpi)erties of dwarf nova EY Cyg and the companion star using an XMM-Newton observation ANDabViAzaNdCeEhS A IN., B SAPLAMCEA NR EŞS.EARCH, cilt.66, sa.5, ss.1139-1146, 2020 (SCI İndekslerine Giren Dergi) III. ABAccLrMeAtiNo nŞ .flows in nonmagnetic white dwarf binaries as observed in X-rays IV. PArDeVfAaNceC:E NS oINv aS PeArCuEp tRiEoSnEsA, RcaCtHa, ccliylts.6m6i, cs sv.1a0r9ia7b-1le1s2 2a,n 2d0 2r0e l(aStCeId İ nsdyesktselmersin: eC Ghiarlelne nDgeersg ii)n the 2020 era ABDALVMANACNE ŞS. IN SPACE RESEARCH, cilt.66, sa.5, ss.1001-1003, 2020 (SCI İndekslerine Giren Dergi) V. XDRisBks structure of cataclysmic variables and broadband noise characteristics in comparison with ABSATLRMOANNO ŞM.ISCHE NACHRICHTEN, cilt.340, sa.4, ss.296-301, 2019 (SCI İndekslerine Giren Dergi) VI. OAvpdtiacna Sl .C, AoKuYnÜteZr Ap.,a Vritnso okfu rUoLvX As. , aAnKdS ATKhEeRir N H., oAsvtd aEnn vHi.r, Foanbmriekna tSs. , iVna NleGevC A 4.,4 A9k0k/ay4a4-8O5ralhan I., BALMAN Ş. VII. SAcSiTeRnOcPeH wYiStIhC AeL-A JOSUTRNOAGLA, Mcil tA.8 7sp5,a scae.1 m, 2i0ss1i9o (nS CfoI rİn MdeekVs-leGreinVe gGairmenm Da-erragyi) astrophysics ADreg Aan gAe.l, ies tA a.,l .Tatischeff V., Grenier I. A. , McEnery J., Mallamaci M., Tavani M., Oberlack U., Hanlon L., Walter R., VIII. AJO UloRnNgA sLe OrFe nHdIGipHit EoNuEsR XGMY MAS-NTReOwPtHonYS oICbSs, ecrilvt.a1t9i,o sns. 1o-f1 0th6e, 2 i0n1te8r (mSCeId İinadtek psloelrainre X GYir Aenr iDergi) MCaOmNuTrHdLaYn NDO. ZT.I ,C BEAS LOMFA TNH EŞ. ,R BOuYrAwLit Az SVT.RONOMICAL SOCIETY, cilt.477, sa.3, ss.4035-4045, 2018 (SCI İndekslerine IX. MGioredni fDyeinrgi )the Standard Disk Model for the Ultraviolet Spectral Analysis of Disk-dominated CGaotdaocnl yPs.,m Siiocn V Ea. rMia. b, Bleaslm. Ia. nT Şh.,e B Nlaoirv Wal.i kPe.s MV Lyrae, BZ Camelopardalis, and V592 Cassiopeiae X. RASeTaRnOaPlyHsYisS IoCfA Lh iJgOhU-RrNesAoLl,u ctilito.8n4 6X,M saM.1-,N 2e0w17to (nS CdI aİntad eokfs lVe2ri4n9e 1G iCreyng nDie urgsii)ng models of collisionally ionized hBoAtL MabAsNo Şr.b, Gerasmsizkan C. XI. XA-SRTAROYN SOPMEYC T&R AASLT RAONPDH YOSPICTSI,C cAilLt.5 P9R8,O 2P0E1R7T (ISECSI İOnFde Aks UleLriXn eI NG iNreGnC D 4er2g5i)8 (M106) ASvTdRanO PHH., YASvIdCaAnL SJ.O, AUKRYNÜAZL ,A c.i, lBt.8A2L8M, AsaN.2 Ş, .2, A01K6S A(KSCEIR İ nNd.,e Okrsalelhrianne IG. Air.en Dergi) XII. PBrAeL-MoAuNtb Şu.rst Chandra observations of the recurrent nova T Pyxidis XIII. SAWSTIRFOTN XO-MRYA Y& IALSLTERSOCPOHPYESI COSB, SciEltR.5V7A2,T 2I0O1N4S ( SOCFI İTnHdEek NslOerVinAe- LGIirKeEn CDAerTgAi)CLYSMIC VARIABLES MV Lyr, BZ CBaAmLM, AN DŞ. , VG5o9d2on C Pa.s, Sion E. M. ASTROPHYSICAL JOURNAL, cilt.794, sa.1, 2014 (SCI İndekslerine Giren Dergi) XIV. Av sdeaanr Hch., Afovdra pne Sr. iKo.d , iAcKitYieÜsZ fAr.o, BmA aL MUALNX Şin. the LINER galaxy NGC 4736 XV. XAMSTMRO-NPEHWYSTICOSN A ONBDS SEPRAVCEA TSCIOIENNSC EO,F c iLlt.U3M52I,N sOa.U1,S s sS.1O2U3R-1C2E8S, 2IN01 N4 E(ASCRIB İnYd GekAsLleArXinIeE GS irNeGnC D 4er3g9i)5, NGC 4736, AKNYDÜ ZN GA.C, K 4a2y5ac8i S., Avdan H., Ozel M. E. , Sonbas E., BALMAN Ş. XVI. XA-SrTaRyO vNaOrMiaICtiAoLn sJO iUnR tNhAeL i,n cnilte.1r4 a5c, csrae.3t,i o20n1 f3lo (wSC oI İfn ddwekasrlef rninoev Gaieren Dergi) ABSATLRMOANNO ŞM.,Y R &ev AnSivTtRseOvP MHY.SICS, cilt.546, 2012 (SCI İndekslerine Giren Dergi) XVII. TBheaer domutobrue rAs.t P o. ,f ONsobovran Ce SJ.S P 0. ,8 P1a0g0e 7K:.0 L3. 0, H5a5k9a+la0 P5. 4J. 7, 1Sc5h w(HarVz CGe. Jt.i ), Rauch T., BALMAN Ş., Evans P. A. , Goad M. R. A, NSTesRsO JN. -O. M, eYt a&l. ASTROPHYSICS, cilt.545, 2012 (SCI İndekslerine Giren Dergi) XVIII. NOREWBITOANL- OPHBSAESREV-RAETSOORLYV EDDA TSAPECTROSCOPY OF THE INTERMEDIATE POLAR FO AQR USING XMM- APeSkToRnO NY.O, BMAICLAMLA JNO UŞ.RNAL, cilt.144, sa.2, 2012 (SCI İndekslerine Giren Dergi) XIX. BXMOUMN-NDEAWRYT OLNAY OEBRSERVATIONS OF THE DWARF NOVA RU Peg IN QUIESCENCE: PROBE OF THE ABSATLRMOAPNH YŞ.S, IGCoAdLo JnO PU.R, SNioAnL ,E c.i lMt.7. ,4 N1e, sas .2J.,, S2c0h1l1eg (eSlC EI. ,İ nBdaerrkestlet rPi.n Ee. G, Sirzekno dDye rPg.i) XX. dOartbaital and spin phase-resolved spectroscopy of the intermediate polar EX Hya using XMM-Newton MPeOkNoTnH YL., YB NALOMTIACNES Ş O.F THE ROYAL ASTRONOMICAL SOCIETY, cilt.411, sa.2, ss.1177-1196, 2011 (SCI İndekslerine XXI. FGrireeqnu Deenrcgyi)-resolved spectroscopy of XB1323-619 using XMM-Newton data: detection of a reflection rBeAgLiMonA Nin Ş .the disc GMiOreNnT DHeLrYg iN)OTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.407, sa.3, ss.1895-1902, 2010 (SCI İndekslerine XXII. ASo snebaarsc Eh., fAoKrY sÜuZp Ae.,r BnAoLvMa ArNem Ş.n, Oanzetls M in. E t.he nearby spiral galaxy M74 (NGC 628) XXIII. TAhSTeR XOMNMOM-NYe &w AtoSTnR dOePtHeYctSiIoCnS, ocifl te.5x1t7e,n 2d0e1d0 e(SmCiIs İsnidoenk sflreormine t hGeir enno Dvaer rgei)mnant of T Pyxidis MBAOLNMTAHNLY Ş .NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.404, sa.1, 2010 (SCI İndekslerine Giren Dergi) XXIV. SBweairftd mobosre rAv. aPt. i,o Onssb oorfn CeS JS. P0.8 , 1P0ag0e7 K:0. 3L.0 , 5S5ch9w+a0r5z 4G7., 1S5tarrfield S., Hakala P., Ness J. -. , BALMAN Ş., Wagner R. M. XXV. AS STTRUODNYO MOIFS CTHHEE N LAOCWHR-IMCHATSESN X, -cRilAt.3Y3 B1,I sNaA.2R, sYs .D15IP6 -S1O59U, R2C0E10S (XSBC I1 İ9nd1e6k-s0le5r3in, eX BGi r1e3n2 D3e-r6g1i)9, X 1624-490 ABANLDM 4AUN 1Ş.746-371 OBSERVED WITH INTEGRAL XXVI. TAhSTeR bOrNoOaMd-ICbAaLn dJO nUoRiNseA Lc,h cailrt.a1c3t8e, rsias.1ti,c sss .o50f -s6e2l,e 2c0te0d9 (aSnCoI mİnadleokussle rXi-nrea Gyi rpeunl sDaerrsg ia)nd soft gamma-ray rKeupleebai tBe.r, sBALMAN Ş. GMiOreNnT DHeLrYg iN)OTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.395, sa.4, ss.2356-2362, 2009 (SCI İndekslerine XXVII. An optical search for supernova remnants in the nearby spiral galaxy NGC 2903 ASoSnTbRaOsN EO.,M AYK Y&Ü AZS AT.R, BOAPHLMYSAINCS Ş, .cilt.493, sa.3, ss.1061-1065, 2009 (SCI İndekslerine Giren Dergi) XXVIII. NVaerwiatotino nasn din I NthTeE dGiRpA pLroperties of the low-mass X-ray binary XB 1254-690 observed with XMM- ATrSiTgRoO MN. ODM. ,Y P &ar AmSaTrR AO. PNH. Y, BSIoCiSri, nc iLlt..,4 M93o,t csha .1C,. , sTsa.1la4v5e-r1a5 7A,. ,2 B0A0L9M (ASCNI Şİn.dekslerine Giren Dergi) XXIX. RPeRk oPeicn (Y1., 9B2A5L)M: AAN C Şh.andra X-ray view GMiOreNnT DHeLrYg iN)OTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.388, sa.2, ss.921-926, 2008 (SCI İndekslerine XXX. TGhelein ion Dcl.i, nBaAtLioMnA Nan Şg.,l Ke izainlodg lmu aUs., sY iolmf athz eA .b, Klaaclekm hcoi lEe., iTno mXTsiEck J 1J.118+480 XXXI. TAhSTeR dOePtHeYctSiIoCnA Lo JfO aU R3N.5A hLr, c pilte.6r4io2d, s ian.1 t, hsse. 4c3la8s-4s4ic2a, l2 n00o6v a( SVCeI lİonrduekms le1r9in9e9 G (iVre3n8 D2e Vrgeil)) and the long-term bBeAhLaMvAioNr Ş o., fR ethtte rN Ao.,v Bao lsi gMh.t curve XXXII. ASnT aRrOcNhOivMaIlC sAtLu dJOyU oRfN eAxLt, ecniltd.1e3d1 X, s-ar.a5y, s es.m26is2s8i-o2n6 3f3ro, 2m0 0c6la (sSsCiIc aİnl daenkdsl erreincue rGrierennt Dneorvgai)e ABDalVmAaNnC ŞE.S IN SPACE RESEARCH, cilt.38, sa.12, ss.2840-2843, 2006 (SCI İndekslerine Giren Dergi) XXXIII. XB-aryakya l oAu., tKbiuzirlosgt lou fU 4., UK i0zi1lo1g5lu+ N6.3, B4A aLnMdA RNO ŞT., SInEa mob Ss.ervations of its optical counterpart V635 Cas XXXIV. CAhSTaRnOdNraO MobY s&e rAvSaTtRioOnP HoYfS tIhCeS, schilte.4ll3 o9,f sNa.o3v, sas .P1e1r3s1e-1i 113940, 12 0(0G5K ( SPCeIr İsnedie)k: sDleertineec tGioirne no Df elorgcia)lized nBoAnLMthAeNrm Ş.al X-ray emission from a miniature supernova remnant XXXV. DASisTcRoOvPeHrYyS oICfA iLrr JaOdUiRaNtiAoLn,- ciniltd.6u2c7e, ds av.2a,r sisa.9ti3o3n-s9 5in2, t2h0e0 5li g(ShCt Ic İunrdveeks olefr itnhee G cilraesns Dicearlg ni)ova V2275 Cyg (N Cyg 2B0al0m1a nN Şo.., Y2ı)lmaz A., Retter A., Saygac T., Esenoglu H. H. GMiorennth Dlye rNgoi)tices of the Royal Astronomical Society, cilt.356, sa.2, ss.773-777, 2005 (SCI Expanded İndekslerine XXXVI.
Load more

Recommended publications
  • The Old Nova CP Puppis: a Carbon Nova and Asynchronous Polar?⋆
    A&A 539, A94 (2012) Astronomy DOI: 10.1051/0004-6361/201117251 & c ESO 2012 Astrophysics The old nova CP Puppis: a carbon nova and asynchronous polar? A. Bianchini1,T.Saygac2, M. Orio3, M. della Valle4, and R. Williams5 1 Department of Astronomy, University of Padova, vicolo dell’Osservatorio 3, 35122 Padova, Italy e-mail: [email protected] 2 Department of Astronomy and Space Sciences, Istanbul University, Istanbul 34119, Turkey 3 INAF – Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, Italy 4 INAF – Osservatorio Astronomico di Napoli, Salita Moiariello 16, 80131 Napoli, Italy 5 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA Received 12 May 2011 / Accepted 21 January 2012 ABSTRACT Context. CP Pup (Nova Pup 1942) showed outburst and quiescent characteristics indicating a very massive white dwarf, yet the standard spectroscopic dynamical analysis assuming an accretion disk yields an extremely low value for the white dwarf mass. However, some physical parameters and the accretion geometry are still poorly known. Aims. The nova was spectroscopically monitored between 1988 and 1996. We analyzed the whole data set in order to re-determine the spectroscopic period and examine its stability. We also looked for chemical anomalies in the spectrum. Methods. We obtained the radial velocity curves for the hydrogen and helium lines from our last better quality 1996 run. The mean 1996 spectrum yields information on the chemical composition of the binary. We also searched the mean period using the multi-year data set. Results. From the radial velocities of our complete data set we derive the most probable mean spectroscopic period and tentatively suggest revised ephemeris.
    [Show full text]
  • Keith Horne: Refereed Publications Papers Submitted: 425. “A
    Keith Horne: Refereed Publications Papers Submitted: 427. “The Lick AGN Monitoring Project 2016: Velocity-Resolved Hβ Lags in Luminous Seyfert Galaxies.” V.U, A.J.Barth, H.A.Vogler, H.Guo, T.Treu, et al. (202?). ApJ, submitted (01 Oct 2021). 426. “Multi-wavelength Optical and NIR Variability Analysis of the Blazar PKS 0027-426.” E.Guise, S.F.H¨onig, T.Almeyda, K.Horne M.Kishimoto, et al. (202?). (arXiv:2108.13386) 425. “A second planet transiting LTT 1445A and a determination of the masses of both worlds.” J.G.Winters, et al. (202?) ApJ, submitted (30 Jul 2021). (arXiv:2107.14737) 424. “A Different-Twin Pair of Sub-Neptunes orbiting TOI-1064 Discovered by TESS, Characterised by CHEOPS and HARPS” T.G.Wilson et al. (202?). ApJ, submitted (12 Jul 2021). 423. “The LHS 1678 System: Two Earth-Sized Transiting Planets and an Astrometric Companion Orbiting an M Dwarf Near the Convective Boundary at 20 pc” M.L.Silverstein, et al. (202?). AJ, submitted (24 Jun 2021). 422. “A temperate Earth-sized planet with strongly tidally-heated interior transiting the M8 dwarf LP 791-18.” M.Peterson, B.Benneke, et al. (202?). submitted (09 May 2021). 421. “The Sloan Digital Sky Survey Reverberation Mapping Project: UV-Optical Accretion Disk Measurements with Hubble Space Telescope.” Y.Homayouni, M.R.Sturm, J.R.Trump, K.Horne, C.J.Grier, Y.Shen, et al. (202?). ApJ submitted (06 May 2021). (arXiv:2105.02884) Papers in Press: 420. “Bayesian Analysis of Quasar Lightcurves with a Running Optimal Average: New Time Delay measurements of COSMOGRAIL Gravitationally Lensed Quasars.” F.R.Donnan, K.Horne, J.V.Hernandez Santisteban (202?) MNRAS, in press (28 Sep 2021).
    [Show full text]
  • Shells Around Southern Novae H
    No. 17 - June 1979 Shells Around Southern Novae H. W. Duerbeck and W. C. Seitter Spencer Jones published in 1931 a bulky volume of Although less spectacular than their big brothers, spectroscopic and visual observations made at the Cape the supernovae, the novae are by no means less Observatory. Another southern observer, J. Hartmann in interesting. They are also much more frequent Buenos Aires, observed the nova spectroscopically and wrote the most concise astronomical paper ever publish­ and several are known in the southern sky. After ed, a telegram senJ to the Astronomische Nachrichten: the initial explosion, a shell expands around the "Nova problem solved; star blows up, bursts." And indeed, nova and may become visible after a while. Drs. when double-star observers examined the postnova two Hilmar Duerbeck and Waltraut Seitter from the Hoher-List Observatory, near Bonn, FRG, recently observed three southern novae. The excellent resolution of the 3.6 m photos makes itpossible to see details in the very faint nova shells that have never been perceived before. The southern sky comprises one of the most fanciful supernova remnants-the extended spider web of the Gum nebula. It harbours also some less spectacular, tiny, astronomically shortlived phenomena: the remnants of near nova explosions. They can be observed for only a few decades after outburst, before they thin out and merge into the interstellar medium. Due to their small size and low surface brightness, they require large telescopes, such as have recently become available in the southern hemi­ sphere. Fortunately, some observing time was granted to us before the above-mentioned disappearances! RR Pictoris Two brilliant novae shone in the southern sky in this century.
    [Show full text]
  • Publications of Variable Star Section, Royal
    J No. 11 (C83)J 4 5 o i o 3 a —i—|—r FIGURE 5 PUBLICATIONS of 7 VARIABLE STAR SEQTI ROYAL ASTRONOMICAL SOCIETY OF NEW ZEALAND 10 to u 11 1% '3 1 liiii o o 0 0 34 NO Nj> • • C -t- T T m to GU JU Mm SGR it Director: Frank M. Bateson P.O. Box 3093, GREERTON, TAURANGA, ft- NEW ZEALAND. i CONTENTS. PAGE THE LIGHT CURVE OF OY CARINAE, 1963 June 15 to 1983 May 31. Frank M. Bateson & A.W. Dodson 1 VISUAL OBSERVATIONS OF THE ECLIPSES OF THE DWARF NOVA OY CARINAE. N.W. Taylor & A.C. Gilmore 14 U HOROLOGII—A NEGLECTED MIRA VARIABLE. C.W. Venimore 22 PHOTOELECTRIC UBV SEQUENCES FOR FOUR SUSPECTED RCB STARS. David Kilkenny 29 PHOTOELECTRIC PHOTOMETRY OF V856 SCORPII & NEARBY SEQUENCE STARS. Brian F. Marino & W.S.G. Walker 31 VISUAL OBSERVATIONS OF V818 SCORPII (Sco X-l) 1974- 1982. Frank M. Bateson & C.W. Venimore 35 THE SEMI-REGULAR VARIABLE, RX RETICULI. A.W. Dodson 45 COLOURS FOR THE VARIABLE STAR V384 CARINAE. Brian F. Marino & W.S.G. Walker 48 REPORT ON SOME NOVAE & SUSPECTED RECURRENT NOVAE. Frank M. Bateson 51 A VISUAL ATLAS OF THE LARGE MAGELLANIC CLOUD. Mati Morel 62 LIGHT CURVE OF NOVA MUSCAE 1983. Frank M. Bateson & A.W. Dodson 65 ASTRONOMICAL RESEARCH LIMITED Frank M. Bateson 69 REPORT OF THE VARIABLE STAR SECTION, ROYAL ASTRONOMICAL SOCIETY OF NEW ZEALAND FOR YEAR ENDED 1983 December 31 70 PUBLISHED BY ASTRONOMICAL RESEARCH LIMITED P.O. BOX 3093, GREERTON TAURANGA, NEW ZEALAND.
    [Show full text]
  • A Remarkable Recurrent Nova in M31: Discovery and Optical/UV Observations of the Predicted 2014 Eruption?,??
    A&A 580, A45 (2015) Astronomy DOI: 10.1051/0004-6361/201526027 & c ESO 2015 Astrophysics A remarkable recurrent nova in M31: Discovery and optical/UV observations of the predicted 2014 eruption?;?? M. J. Darnley1, M. Henze2, I. A. Steele1, M. F. Bode1, V. A. R. M. Ribeiro3, P. Rodríguez-Gil4;5, A. W. Shafter6, S. C. Williams1, D. Baer6, I. Hachisu7, M. Hernanz8, K. Hornoch9, R. Hounsell10, M. Kato11, S. Kiyota12, H. Kucákovᡠ13, H. Maehara14, J.-U. Ness2, A. S. Piascik1, G. Sala15;16, I. Skillen17, R. J. Smith1, and M. Wolf13 1 Astrophysics Research Institute, Liverpool John Moores University, IC2 Liverpool Science Park, Liverpool, L3 5RF, UK e-mail: [email protected] 2 European Space Astronomy Centre, PO Box 78, 28691 Villanueva de la Cañada, Madrid, Spain 3 Department of Astrophysics/IMAPP, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands 4 Instituto de Astrofísica de Canarias, Vía Láctea, s/n, La Laguna, 38205 Santa Cruz de Tenerife, Spain 5 Departamento de Astrofísica, Universidad de La Laguna, La Laguna, 38206 Santa Cruz de Tenerife, Spain 6 Department of Astronomy, San Diego State University, San Diego, CA 92182, USA 7 Department of Earth Science and Astronomy, College of Arts and Sciences, The University of Tokyo, 3-8-1 Komaba, Meguro-ku, 153-8902 Tokyo, Japan 8 Institut de Ciències de l’Espai (CSIC-IEEC), Campus UAB, Fac. Ciències, 08193 Bellaterra, Spain 9 Astronomical Institute, Academy of Sciences, 251 65 Ondrejov,ˇ Czech Republic 10 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore,
    [Show full text]
  • Interacting Binaries No
    Interacting Binaries No. 32, January 28th 2009 An Electronic Newsletter Editors: Boris T. Gansicke¨ Dept. of Physics, University of Warwick, Coventry CV4 7AL, UK Andrew J. Norton Dept. of Physics & Astronomy, The Open University, Milton Keynes MK7 6AA, UK [email protected], http://www.warwick.ac.uk/staff/Boris.Gaensicke/IBNews/ Contents 1 Editorial 2 2 Abstracts of refereed papers 3 – Two new intermediate polars with a soft X-ray component Anzolin et al. ................ 3 – RXTE determination of the intermediate polar status of XSS J00564+4548, IGR J17195–4100, and XSS J12270–4859 Butters et al. .................................... 3 – Circular polarization survey of intermediate polars I. Northern targets in the range 17h<R.A.<23h Butters et al. ..................................... 4 – RXTE confirmation of the intermediate polar status of IGR J15094–6649 Butters et al. ........ 4 – ULTRACAM observations of two accreting white dwarf pulsators Copperwheat et al. ......... 5 – On the apsidal motion of BP Vulpeculae Csizmadia et al. ........................ 6 – How many cataclysmic variables are crossing the period gap? A test for the disruption of magnetic braking Davis et al. ........................................... 6 – Optical spectroscopy and photometry of SAX J1808.4−3658 in outburst Elebert et al. ......... 7 – The spectroscopic orbit and the geometry of R Aqr Gromadzki & Mikolajewska ............ 7 – XMM-Newton and Optical Observations of Cataclysmic Variables from SDSS Hilton et al. ...... 8 – New Complexities in the Low-State line profiles of AM Herculis Kafka et al. .............. 8 – Observations of V592 Cas - An Outflow at Optical Wavelengths Kafka et al. .............. 9 – Variation of fluxes of RR Tel emission lines measured in 2000 with respect to 1996 Kotnik-Karuza et al.
    [Show full text]
  • Observer's Handbook 1988
    OBSERVER’S HANDBOOK 1988 EDITOR: ROY L. BISHOP THE ROYAL ASTRONOMICAL SOCIETY OF CANADA CONTRIBUTORS AND ADVISORS A l a n H. B a t t e n , Dominion Astrophysical Observatory, 5071 W. Saanich Road, Victoria, BC, Canada V8X 4M6 (The Nearest Stars). L a r r y D. B o g a n , Department of Physics, Acadia University, Wolfville, NS, Canada B0P 1X0 (Configurations of Saturn’s Satellites). T e r e n c e D ic k i n s o n , Yarker, ON, Canada K0K 3N0 (The Planets). D a v id W. D u n h a m , International Occultation Timing Association, P.O. Box 7488, Silver Spring, MD 20907, U.S.A. (Lunar and Planetary Occultations). A l a n D y e r , Edmonton Space Sciences Centre, 11211-142 St., Edmonton, AB, Canada T5M 4A1 (Messier Catalogue, Deep-Sky Objects). F r e d E s p e n a k , Planetary Systems Branch, NASA-Goddard Space Flight Centre, Greenbelt, MD, U.S.A. 20771 (Eclipses and Transits). M a r ie F id l e r , 23 Lyndale D r., Willowdale, ON, Canada M2N 2X9 (Observatories and Planetaria). V ic t o r G a i z a u s k a s , C h r is t ie D o n a l d s o n , T e d K e n n e l l y , Herzberg Institute of Astrophysics, National Research Council, Ottawa, ON, Canada K1A 0R6 (Solar Activity). R o b e r t F. G a r r is o n , David Dunlap Observatory, University of Toronto, Box 360, Richmond Hill, ON, Canada L4C 4Y6 (The Brightest Stars).
    [Show full text]
  • INES Access Guide No. 3 Classical Novae
    INES Access Guide No. 3 Classical Novae Compiled by: Angelo Cassatella Consiglio Nazionale delle Ricerche IFSI (Roma) and Rosario Gonz´alez-Riestra XMM Science Operations Centre ESAC (Madrid) and Pierluigi Selvelli Consiglio Nazionale delle Ricerche IASF (Roma), INAF-OAT (Trieste) Scientific Coordinator for the INES Acess Guides Dr. Willem Wamsteker 1 2 FOREWORD The INES Access Guides The International Ultraviolet Explorer (IUE) Satellite (launched on 26 January 1978 and in or- bit until September 1996) Project was a collaboration between NASA, ESA and the PPARC. The IUE Spacecraft and instruments were operated in a Guest Observer mode to allow Ultraviolet Spec- trophotometry at two resolutions in the wavelength range from 115nm to 320nm: low resolution ∆λ/λ=300 (≈1000 km sec−1) and a high resolution mode ∆λ/λ=10000 (≈19 km sec−1). The IUE S/C, its scientific instruments as well as the data acquisition and reduction procedures, have been described in “Exploring the Universe with the IUE Satellite”, Part I, Part VI and Part VII (ASSL, volume 129, Eds. Y. Kondo, W. Wamsteker, M. Grewing, Kluwer Acad. Publ. Co.). A complete overview of the IUE Project is given in the conference proceedings of the last IUE Conference “Ultra- violet Astrophysics beyond the IUE Final Archive” (ESA SP-413, 1998, Eds. W. Wamsteker and R. Gonz´alezRiestra) and in “IUE Spacecraft Operations Final Report” (ESA SP-1215, 1997, A. P´erez Calpena and J. Pepoy). Additional information on the IUE Project and its data Archive INES can be found at URL http://sdc.laeff.esa.es. From the very beginning of the project, it was expected that the archival value of the data obtained with IUE would be very high.
    [Show full text]
  • CP Puppis: Another V1500 Cyg?
    CP Puppis: Another V1500 Cyg? D. O'Donoghue and B. Warner Dept. of Astronomy, Univ. of Cape Town. W. Wargau Dept. of Maths, Appl. Maths and Autonomy, Univ. of South Africa. A.D. Grauer Dept. of Physics and Astronomy, Univ. of Arkansas at Little Rock. 1. Introduction As first pointed out by Warner (1985), the overall properties of CP Pup and V1500 Cyg are very similar: both were very fast, very large amplitude novae with ~0.3 mag photometric humps at roughly the orbital period. Neither variation is strictly periodic (Patterson 1979; Warner 1985). Variable circu­ lar polarization (with period slightly different from the orbital period) has been found in V1500 Cyg showing that its white dwarf is strongly magnetic and has broken synchronism with the secondary star (Stockman, Schmidt & Lamb 1988). In contrast, no circular polarization has been found in CP Pup. Nonetheless, does the slight difference between the photometric and spectroscopic periods indicate it is also a magnetic system (Warner 1985; Bianchini et al. 1985a)? New photometric and spectroscopic data for CP Pup are reported which resolve the aliases and confusion in the periods found by Bianchini et al. (1985a,b), Warner (1985) and Duerbeck et al. (1987) and allow an examination of the evidence for its magnetic nature. 2. Observations The new data comprise: (i) 48 hrs of white light high speed photometry obtained during January 1986 and March 1988 at SAAO and Mt. Stromlo; (ii) time-resolved spectra (3600-5400A) during April 1985 and March 1988. The new photometry shows the -1.5 hr modulation discovered by Warner (1985), but with a large range in amplitude, from 40% to invisibility, suggestive of beating of two or more unresolved frequen­ cies.
    [Show full text]
  • Observer's Handbook 1981
    OBSERVER’S HANDBOOK 1 9 8 1 EDITOR: JOHN R. PERCY ROYAL ASTRONOMICAL SOCIETY OF CANADA CONTRIBUTORS AND ADVISORS A l a n H. B a t t e n , Dominion Astrophysical Observatory, Victoria, B.C., Canada V8X 3X3 (The Nearest Stars). Terence Dickinson, Editor, Star and Sky, 44 Church Lane, Westport, Conn. 06880 (The Planets). Alan Dyer, Queen Elizabeth Planetarium, 10004-104 Ave., Edmonton, Alta. T5J 0K 1 (Messier Catalogue, Deep-Sky Objects). M arie Fidler, Royal Astronomical Society of Canada, 124 Merton St., Toronto, Ont., Canada M4S 2Z2 (Observatories and Planetariums). V ictor Gaizauskas, Herzberg Institute of Astrophysics, National Research Council, Ottawa, Ont., Canada K1A 0R6 (Sunspots). J o h n A. G a l t , Dominion Radio Astrophysical Observatory, Penticton, B.C., Canada V2A 6K3 (Radio Sources). Ian H alliday, Herzberg Institute of Astrophysics, National Research Council, Ottawa, Ont., Canada K1A 0R6 (Miscellaneous Astronomical Data). H e l e n S. H o g g , David Dunlap Observatory, University of Toronto, Richmond Hill, Ont., Canada L4C 4Y6 (Foreword). D o n a l d A. M a c R a e , David Dunlap Observatory, University of Toronto, Richmond Hill, Ont., Canada L4C 4Y6 (The Brightest Stars). B r i a n G. M a r s d e n , Smithsonian Astrophysical Observatory, Cambridge, Mass., U.S.A. 02138 (Comets, Minor Planets). J a n e t A. M a t t e i , American Association of Variable Star Observers, 187 Concord Ave., Cambridge, Mass. U.S.A. 02138 (Variable Stars). P e t e r M. M i l l m a n , Herzberg Institute of Astrophysics, National Research Council, Ottawa, Ont., Canada K1A 0R6 (Meteors, Fireballs and Meteorites).
    [Show full text]
  • Observer's Handbook 1979
    OBSERVER’S HANDBOOK 1979 EDITOR: JOHN R. PERCY ROYAL ASTRONOMICAL SOCIETY OF CANADA THE ORIGINS OF THE ROYAL ASTRONOMICAL SOCIETY OF CANADA In the mid-nineteenth century, in the bustling Lake Ontario port city of Toronto, there were no professional astronomers. However, many inhabitants of the city were keenly interested in sciences and current developments in them. King’s College, which grew into the University of Toronto, had been started in 1842. In 1849 it had 36 undergraduates attending, and had graduated a total of 55 students in the three faculties of arts, law and medicine. The Toronto Magnetic Observatory had been established in 1840. Its early directors and observers were officers and soldiers in garrison. Some of them, such as Captain J. F. Lefroy, contributed much to the cul­ tural life of the city. Out of this body of interest came the Canadian Institute estab­ lished in 1849 “to promote those pursuits which are calculated to refine and exalt a people” . Besides holding weekly meetings, the Canadian Institute accumulated an out­ standing library. There many hours were spent in study by Andrew Elvins who had come to Canada from Cornwall in 1844. In 1860 he moved to Toronto, with a population then of 44,000, and became chief cutter in a well known clothing store on King Street. While the Canadian Institute held discussion meetings of all sciences, Elvins wished to concentrate on astronomy. For this purpose he gathered together a few like-minded friends. On December 1, 1868 The Toronto Astronomical Club met for the first time, at the Elvins’ home, “having for its object the aiding of each other in the pursuit of astronomical knowledge”.
    [Show full text]
  • Annual Report Publications 2012
    Publications Publications in refereed journals based on ESO data (2012) The ESO Library maintains the ESO Telescope Bibliography (telbib) and is responsible for providing paper-based statistics. Access to the database for the years 1996 to present as well as information on basic publication statistics are available through the public interface of telbib (http://telbib.eso.org) and from the “Basic ESO Publication Statistics” document (http://www.eso.org/sci/libraries/edocs/ESO/ESOstats.pdf), respectively. In the list below, only those papers are included that are based on data from ESO facilities for which observing time is evaluated by the Observing Programmes Committee (OPC). Publications that use data from non-ESO telescopes or observations obtained during ‘private’ observing time are not listed here. Acharova, I.A., Mishurov, Y.N. & Kovtyukh, V.V. 2012, Alaghband-Zadeh, S., Chapman, S.C., Swinbank, A.M., Galactic restrictions on iron production by various Smail, I., Harrison, C.M., Alexander, D.M., Casey, types of supernovae, MNRAS, 420, 1590 C.M., Davé, R., Narayanan, D., Tamura, Y. & Umehata, Adami, C., Jouvel, S., Guennou, L., Le Brun, V., Durret, H. 2012, Integral field spectroscopy of 2.0< z<2.7 F., Clement, B., Clerc, N., Comerón, S., Ilbert, O., Lin, submillimetre galaxies: gas morphologies and Y., Russeil, D. & Seemann, U. 2012, Comparison of kinematics, MNRAS, 424, 2232 the properties of two fossil groups of galaxies with the Albrecht, S., Winn, J.N., Butler, R.P., Crane, J.D., normal group NGC 6034 based on multiband imaging Shectman, S.A., Thompson, I.B., Hirano, T. & and optical spectroscopy, A&A, 540, 105 Wittenmyer, R.A.
    [Show full text]