Sommaire Des Annexes

Total Page:16

File Type:pdf, Size:1020Kb

Sommaire Des Annexes Liste des publications 2001-2003 Sommaire des annexes Liste des publications 2001 - 2003_____________________________________________ 73 Refereed Journal Papers _______________________________________________________ 73 2001______________________________________________________________________________ 73 2002______________________________________________________________________________ 76 2003______________________________________________________________________________ 78 Conference Papers ____________________________________________________________ 83 2001______________________________________________________________________________ 83 2002______________________________________________________________________________ 89 2003______________________________________________________________________________ 93 Non-Refereed Journal Papers ___________________________________________________ 98 2002______________________________________________________________________________ 98 2003______________________________________________________________________________ 99 Livres ______________________________________________________________________ 101 2002_____________________________________________________________________________ 101 2003_____________________________________________________________________________ 101 Personnel du SAp au 1er janvier 2004 _________________________________________ 102 Légende ____________________________________________________________________ 102 Les activités d'interprétation ___________________________________________________ 102 Les activités d'instrumentation spatiale __________________________________________ 103 Membres de Conseils scientifiques Nationaux et Internationaux ___________________ 106 Visiteurs ________________________________________________________________ 107 Organisation de conférences ________________________________________________ 110 Thèses __________________________________________________________________ 111 Enseignement ____________________________________________________________ 113 Participation à des jurys de thèses____________________________________________ 115 Activités de vulgarisation ___________________________________________________ 117 Service d'Astrophysique 2001-2003 DSM - DAPNIA 72 Liste des publications 2001-2003 Liste des publications 2001 - 2003 11. Bonnet-Bidaud, J. M., Mouchet, M., de Martino, D., Matt, Refereed Journal Papers G., Motch, C., 2001, "The white dwarf revealed in the intermediate polar V709 Cassiopeiae", A&A, 374, 1003- 1008 2001 12. Bontemps, S., André, P., Kaas, A. A., Nordh, L., Olofsson, 1. Afonso, C., Albert, J. N., Andersen, J., Ansari, R., Aubourg, G., Huldtgren, M., Abergel, A., Blommaert, J., Boulanger, É., Bareyre, P., Bauer, F., Blanc, G., Bouquet, A., Char, S., F., Burgdorf, M., Cesarsky, C. J., Cesarsky, D., Copet, E., Charlot, X., Couchot, F., Coutures, C., Derue, F., Ferlet, R., Davies, J., Falgarone, E., Lagache, G., Montmerle, T., Fouqué, P., Glicenstein, J. F., Goldman, B., Gould, A., Pérault, M., Persi, P., Prusti, T., Puget, J. L., Sibille, F. , Graff, D., Gros, M., Haissinski, J., Hamilton, J. C., Hardin, 2001, "ISOCAM observations of the rho Ophiuchi cloud: D., de Kat, J., Kim, A., Lasserre, T., LeGuillou, L., Luminosity and mass functions of the pre-main sequence Lesquoy, É., Loup, C., Magneville, C., Mansoux, B., embedded cluster", A&A, 372, 173-194 Marquette, J. B., Maurice, É., Milsztajn, A., Moniez, M., 13. Bouchet, L., Roques, J. P., Ballet, J., Goldwurm, A., Paul, Palanque-Delabrouille, N., Perdereau, O., Prévot, L., J., 2001, "The SIGMA/Granat Telescope: Calibration and Regnault, N., Rich, J., Spiro, M., Vidal-Madjar, A., Data Reduction", ApJ, 548, 990-1009 Vigroux, L., Zylberajch, S., The EROS collaboration, 2001, 14. Braine, J., Duc, P.-A., Lisenfeld, U., Charmandaris, V., "Photometric constraints on microlens spectroscopy of Vallejo, O., Leon, S., Brinks, E., 2001, "Abundant EROS-BLG-2000-5", A&A, 378, 1014-1023 molecular gas in tidal dwarf galaxies: On-going galaxy 2. Arnaud, M., Aghanim, N., Gastaud, R., Neumann, D. M., formation", A&A, 378, 51-69 Lumb, D., Briel, U., Altieri, B., Ghizzardi, S., Mittaz, J., 15. Briel, U. G., Henry, J. P., Lumb, D. H., Arnaud, M., Sasseen, T. P., Vestrand, W. T., 2001, "XMM-Newton Neumann, D., Aghanim, N., Gastaud, R., Mittaz, J. P. D., observation of the Coma Galaxy cluster. The temperature Sasseen, T. P., Vestrand, W. T., 2001, "A mosaic of the structure in the central region", A&A, 365, L67-L73 Coma cluster of galaxies with XMM-Newton", A&A, 365, 3. Arnaud, M., Neumann, D. M., Aghanim, N., Gastaud, R., L60-L66 Majerowicz, S., Hughes, J. P., 2001, "Measuring cluster 16. Caunt, S. E., Tagger, M., 2001, "Numerical simulations of temperature profiles with XMM/EPIC", A&A, 365, L80- the accretion-ejection instability in magnetised accretion L86 disks", A&A, 367, 1095-1111 4. Audard, M., Behar, E., Güdel, M., Raassen, A. J. J., 17. Charnoz, S., Brahic, A., 2001, "Long-term collisional Porquet, D., Mewe, R., Foley, C. R., Bromage, G. E. , 2001, evolution of a dissipative particle disc perturbed by a giant- "The XMM-Newton view of stellar coronae: High- planet embryo", A&A, 375, L31-L34 resolution X-ray spectroscopy of Capella", A&A, 365, 18. Charnoz, S., Brahic, A., Ferrari, C., Grenier, I., Roddier, F., L329-L335 Thébault, P., 2001, "Detection of arcs in Saturn's F ring 5. Böhringer, H., Belsole, E., Kennea, J., Matsushita, K., during the 1995 Sun ring-plane crossing", A&A, 365, 214- Molendi, S., Worrall, D. M., Mushotzky, R. F., Ehle, M., 221 Guainazzi, M., Sakelliou, I., Stewart, G., Vestrand, W. T., 19. Charnoz, S., Thébault, P., Brahic, A., 2001, "Short-term Dos Santos, S., 2001, "XMM-Newton observations of M 87 collisional evolution of a disc perturbed by a giant-planet and its X-ray halo", A&A, 365, L181-L187 embryo", A&A, 373, 683-701 6. Böhringer, H., Schuecker, P., Guzzo, L., Collins, C. A., 20. Chary, R., Elbaz, D., 2001, "Interpreting the Cosmic Voges, W., Schindler, S., Neumann, D. M., Cruddace, R. Infrared Background: Constraints on the Evolution of the G., De Grandi, S., Chincarini, G., Edge, A. C., Dust-enshrouded Star Formation Rate", ApJ, 556, 562-581 MacGillivray, H. T., Shaver, P., 2001, "The ROSAT-ESO 21. Chaty, S., Rodríguez, L. F., Mirabel, I. F., Geballe, T. R., flux limited X-ray (REFLEX) galaxy cluster survey. I. The Fuchs, Y., Claret, A., Cesarsky, C. J., Cesarsky, D., 2001, construction of the cluster sample", A&A, 369, 826-850 "A search for possible interactions between ejections from 7. Beaulieu, J.-P., de Wit, W. J., Lamers, H. J. G. L. M., GRS 1915+105 and the surrounding interstellar medium", Marquette, J.-B., Coutures, C., Leisy, P., Totor, S., A&A, 366, 1035-1046 Palanque-Delabrouille, N., Afonso, C., Alard, C., Albert, J. 22. Cui, W., Schulz, N. S., Baganoff, F. K., Bautz, M. W., N., Andersen, J., Ansari, R., Aubourg, É., Bareyre, P., Doty, J. P., Garmire, G. P., Mirabel, I. F., Ricker, G. R., Bauer, F., Blanc, G., Charlot, X., Couchot, F., Derue, F., Rodríguez, L. F., Taylor, S. C. , 2001, "Peculiar Extended Ferlet, R., Glicenstein, P. F. J. F., Goldman, B., Graff, D., X-Ray Emission around the “Radio-loud” Black Hole Gros, M., Haissinski, J., Hamilton, J. C., Hardin, D., de Kat, Candidate 1E 1740.7-2942", ApJ, 548, 394-400 J., Lasserre, T., Lesquoy, É., Loup, C., Magneville, C., 23. Decourchelle, A., Sauvageot, J. L., Audard, M., Mansoux, B., Maurice, É., Milsztajn, A., Moniez, M., Aschenbach, B., Sembay, S., Rothenflug, R., Ballet, J., Perdereau, O., Prévot, L., Regnault, N., Rich, J., Spiro, M., Stadlbauer, T., West, R. G., 2001, "XMM-Newton Vidal-Madjar, A., Vigroux, L., Zylberajch, S., 2001, "Blue observation of the Tycho supernova remnant", A&A, 365, irregular variable stars in the Small Magellanic Cloud from L218-L224 EROS2: Herbig Ae/Be or classical Be stars?", A&A, 380, 24. Derue, F., Afonso, C., Alard, C., Albert, J.-N., Andersen, J., 168-176 Ansari, R., Aubourg, É., Bareyre, P., Bauer, F., Beaulieu, 8. Belsole, E., Sauvageot, J. L., Böhringer, H., Worrall, D. M., J.-P., Blanc, G., Bouquet, A., Char, S., Charlot, X., Matsushita, K., Mushotzky, R. F., Sakelliou, I., Molendi, S., Couchot, F., Coutures, C., Ferlet, R., Fouqué, P., Ehle, M., Kennea, J., Stewart, G., Vestrand, W. T., 2001, Glicenstein, J.-F., Goldman, B., Gould, A., Graff, D., Gros, "An XMM-Newton study of the sub-structure in M 87's M., Haïssinski, J., Hamilton, J.-C., Hardin, D., de Kat, J., halo", A&A, 365, L188-L194 Kim, A., Lasserre, T., Le Guillou, L., Lesquoy, É., Loup, 9. Bocchino, F., Warwick, R. S., Marty, P., Lumb, D., Becker, C., Magneville, C., Mansoux, B., Marquette, J.-B., Maurice, W., Pigot, C., 2001, "The X-ray nebula of the filled center É., Milsztajn, A., Moniez, M., Palanque-Delabrouille, N., supernova remnant 3C 58 and its interaction with the Perdereau, O., Prévot, L., Regnault, N., Rich, J., Spiro, M., environment", A&A, 369, 1078-1087 Vidal-Madjar, A., Vigroux, L., Zylberajch, S., 2001, 10. Bonnet-Bidaud, J. M., Haberl, F., Ferrando, P., Bennie, P. "Observation of microlensing toward the galactic spiral J., Kendziorra, E., 2001, "The eclipsing bursting X-ray arms. EROS II 3 year survey", A&A, 373, 126-138 binary EXO 0748-676 revisited by XMM-Newton", A&A, 25. Digel, S. W., Grenier, I. A., Hunter, S. D., Dame, T. M., 365, L282-L287 Thaddeus, P., 2001, "EGRET Observations of Monoceros: 73 DSM - DAPNIA Service d'Astrophysique 2001-2003 Liste des publications 2001-2003 Diffuse Gamma-Ray Emission in the Outer Galaxy", ApJ, 46. Grosso, N., Alves, J.,
Recommended publications
  • FY08 Technical Papers by GSMTPO Staff
    AURA/NOAO ANNUAL REPORT FY 2008 Submitted to the National Science Foundation July 23, 2008 Revised as Complete and Submitted December 23, 2008 NGC 660, ~13 Mpc from the Earth, is a peculiar, polar ring galaxy that resulted from two galaxies colliding. It consists of a nearly edge-on disk and a strongly warped outer disk. Image Credit: T.A. Rector/University of Alaska, Anchorage NATIONAL OPTICAL ASTRONOMY OBSERVATORY NOAO ANNUAL REPORT FY 2008 Submitted to the National Science Foundation December 23, 2008 TABLE OF CONTENTS EXECUTIVE SUMMARY ............................................................................................................................. 1 1 SCIENTIFIC ACTIVITIES AND FINDINGS ..................................................................................... 2 1.1 Cerro Tololo Inter-American Observatory...................................................................................... 2 The Once and Future Supernova η Carinae...................................................................................................... 2 A Stellar Merger and a Missing White Dwarf.................................................................................................. 3 Imaging the COSMOS...................................................................................................................................... 3 The Hubble Constant from a Gravitational Lens.............................................................................................. 4 A New Dwarf Nova in the Period Gap............................................................................................................
    [Show full text]
  • Nova Report 2006-2007
    NOVA REPORTNOVA 2006 - 2007 NOVA REPORT 2006-2007 Illustration on the front cover The cover image shows a composite image of the supernova remnant Cassiopeia A (Cas A). This object is the brightest radio source in the sky, and has been created by a supernova explosion about 330 year ago. The star itself had a mass of around 20 times the mass of the sun, but by the time it exploded it must have lost most of the outer layers. The red and green colors in the image are obtained from a million second observation of Cas A with the Chandra X-ray Observatory. The blue image is obtained with the Very Large Array at a wavelength of 21.7 cm. The emission is caused by very high energy electrons swirling around in a magnetic field. The red image is based on the ratio of line emission of Si XIII over Mg XI, which brings out the bi-polar, jet-like, structure. The green image is the Si XIII line emission itself, showing that most X-ray emission comes from a shell of stellar debris. Faintly visible in green in the center is a point-like source, which is presumably the neutron star, created just prior to the supernova explosion. Image credits: Creation/compilation: Jacco Vink. The data were obtained from: NASA Chandra X-ray observatory and Very Large Array (downloaded from Astronomy Digital Image Library http://adil.ncsa.uiuc. edu). Related scientific publications: Hwang, Vink, et al., 2004, Astrophys. J. 615, L117; Helder and Vink, 2008, Astrophys. J. in press.
    [Show full text]
  • [Astro-Ph.IM] 5 Nov 2017 INTEGRAL Nodrt Rgesi Hsfil,T Sals Hc R H Technolog Universe
    Noname manuscript No. (will be inserted by the editor) Hard X–ray/Soft gamma–ray experiments and missions: overview and prospects Erica Cavallari · Filippo Frontera Received: date / Accepted: date Abstract Starting from 1960s, a great number of missions and experiments have been performed for the study of the high–energy sky. This review gives a wide vision of the most important space missions and balloon experiments that have operated in the 10–600 keV band, a crucial window for the study of the most energetic and violent phenomena in the Universe. Thus it is important to take the stock of the achievements to better establish what we have still to do with future missions in order to progress in this field, to establish which are the technologies required to solve the still open issues and to extend our knowledge of the Universe. Keywords high-energy astrophysics · hard X-ray astronomy · space missions · balloon experiments 1 Introduction It is recognized that hard X–ray/soft gamma–ray astronomy (10–600 keV) is a crucial window for the study of the most energetic and violent events in the Universe. An increasing number of missions devoted to observations in this band or including instruments specifically devoted to perform hard X–ray observations have been performed (e.g., BeppoSAX , Rossi XTE) or are still operational (e.g., INTEGRAL, Swift, Fermi). Actually in the remote past this was only considered an ancillary energy band. The bands which were considered key for astrophysical observations were the 2–10 keV band, also dubbed classic en- ergy band, and the soft X–ray band (≤ 2 keV).
    [Show full text]
  • SIMULTANEOUS Nustar/CHANDRA OBSERVATIONS of the BURSTING PULSAR GRO J1744-28 DURING ITS THIRD REACTIVATION
    SIMULTANEOUS NuSTAR/CHANDRA OBSERVATIONS OF THE BURSTING PULSAR GRO J1744-28 DURING ITS THIRD REACTIVATION The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Younes, G., C. Kouveliotou, B. W. Grefenstette, J. A. Tomsick, A. Tennant, M. H. Finger, F. Fürst, et al. “SIMULTANEOUS NuSTAR/ CHANDRA OBSERVATIONS OF THE BURSTING PULSAR GRO J1744-28 DURING ITS THIRD REACTIVATION.” The Astrophysical Journal 804, no. 1 (April 29, 2015): 43. © 2015 The American Astronomical Society As Published http://dx.doi.org/10.1088/0004-637x/804/1/43 Publisher IOP Publishing Version Final published version Citable link http://hdl.handle.net/1721.1/98366 Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. The Astrophysical Journal, 804:43 (16pp), 2015 May 1 doi:10.1088/0004-637X/804/1/43 © 2015. The American Astronomical Society. All rights reserved. SIMULTANEOUS NuSTAR/CHANDRA OBSERVATIONS OF THE BURSTING PULSAR GRO J1744-28 DURING ITS THIRD REACTIVATION G. Younes1,2, C. Kouveliotou3,2, B. W. Grefenstette4, J. A. Tomsick5, A. Tennant3,2, M. H. Finger1,2, F. Fürst4, K. Pottschmidt6,7, V. Bhalerao8, S. E. Boggs5, L. Boirin9, D. Chakrabarty10, F. E. Christensen11, W. W. Craig5,12, N. Degenaar13, A. C. Fabian14, P. Gandhi15,E.Göğüş16, C. J. Hailey17, F. A. Harrison4, J. A. Kennea18, J. M. Miller11, D. Stern19, and W. W. Zhang20 1 Universities Space Research Association,
    [Show full text]
  • 7.5 X 11.5.Doubleline.P65
    Cambridge University Press 978-0-521-75618-1 - High Energy Astrophysics, Third Edition Malcolm S. Longair Index More information Name index Abell, George, 99, 101 Cappelluti, Nico, 729 Abraham, Robert, 733 Carter, Brandon, 434 Abramovitz, Milton, 206, 209 Caswell, James, 226 Adams, Fred, 353, 369 Cavaliere, Alfonso, 110 Amsler, Claude, 275 Cesarsky, Catherine, 187, 189 Anderson, Carl, 29, 30, 163 Challinor, Anthony, 115, 259 Arnaud, Monique, 110 Chandrasekhar, Subrahmanyan, 302, 429, 434, Arnett, David, 386 455 Arzoumanian, Zaven, 420 Charlot, Stephane,´ 729, 730, 747 Auger, Pierre, 29 Chwolson, O., 117 Cimatti, Andrea, 736, 748 Babbedge, T., 740 Clayton, Donald, 386 Backer, Donald, 417, 418 Clemmow, Phillip, 267 Bahcall, John, 55, 57, 58 Colless, Matthew, 108, 109 Bahcall, Neta, 105 Compton, Arthur, 231 Balbus, Steven, 455 Cordes, James, 420 Band, David, 264 Cowie, Lennox, 733, 736, 743, 745 Barger, Amy, 745 Cox, Donald, 357 Beckwith, Steven, 737, 744 Becquerel, Henri, 146 Damon, Paul, 297 Bekefi, George, 193 Davies, Rodney, 376 Bell(-Burnell), Jocelyn, 19, 406 Davis, Leverett, 373 Bennett, Charles, 16 Davis, Raymond, 32, 54, 55 Bethe, Hans, 57, 163, 166, 175 de Vaucouleurs, Gerard,´ 77, 78 Bignami, Giovanni, 197 Dermer, Charles, 505 Binney, James, 106, 153 Deubner, Franz-Ludwig, 51 Blaauw, Adriaan, 754 Diehl, Roland, 287 Blackett, Patrick, 29 Dirac, Adrian, 29 Blain, Andrew, 743 Djorgovski, George, 88 Bland-Hawthorn, Jonathan, 733 Dougherty, John, 267 Blandford, Roger, 251 Draine, Bruce, 351, 372, 373, 375, Blumenthal, George, 163, 175,
    [Show full text]
  • The Iso Handbook
    THE ISO HANDBOOK Volume I: ISO – Mission & Satellite Overview Martin F. Kessler1,2, Thomas G. M¨uller1,4, Kieron Leech 1, Christophe Arviset1, Pedro Garc´ıa-Lario1, Leo Metcalfe1, Andy M. T. Pollock1,3, Timo Prusti1,2 and Alberto Salama1 SAI-2000-035/Dc, Version 2.0 November, 2003 1 ISO Data Centre, Science Operations and Data Systems Division Research and Scientific Support Department of ESA, Villafranca del Castillo, P.O. Box 50727, E-28080 Madrid, Spain 2 ESTEC, Science Operations and Data Systems Division Research and Scientific Support Department of ESA, Keplerlaan 1, Postbus 299, 2200 AG Noordwijk, The Netherlands 3 Computer & Scientific Co. Ltd., 230 Graham Road, Sheffield S10 3GS, England 4 Max-Planck-Institut f¨ur extraterrestrische Physik, Giessenbachstraße, D-85748 Garching, Germany ii Document Information Document: The ISO Handbook Volume: I Title: ISO - Mission & Satellite Overview Reference Number: SAI/2000-035/Dc Issue: Version 2.0 Issue Date: November 2003 Authors: M.F. Kessler, T. M¨uller, K. Leech et al. Editors: T. M¨uller, J. Blommaert & P. Garc´ıa-Lario Web-Editor: J. Matagne Document History The ISO Handbook, Volume I: ISO – Mission & Satellite Overview is mainly based on the following documents: • The ISO Handbook, Volume I: ISO – Mission Overview, Kessler M.F., M¨uller T.G., Arviset C. et al., earlier versions, SAI-2000-035/Dc. • The ISO Handbook, Volume II: ISO – The Satellite and its Data, K. Leech & A.M.T. Pollock, earlier versions, SAI-99-082/Dc. • The following ESA Bulletin articles: The ISO Mission – A Scientific Overview, M.F. Kessler, A.
    [Show full text]
  • Kasliwal Phd Thesis
    Bridging the Gap: Elusive Explosions in the Local Universe Thesis by Mansi M. Kasliwal Advisor Professor Shri R. Kulkarni In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy California Institute of Technology Pasadena, California 2011 (Defended April 26, 2011) ii c 2011 Mansi M. Kasliwal All rights Reserved iii Acknowledgements The first word that comes to my mind to describe my learning experience at Caltech is exhilarating. I have no words to thank my “Guru”, Professor Shri Kulkarni. Shri taught me the “Ps” necessary to Pursue the Profession of a Professor in astroPhysics. In addition to Passion & Perseverance, I am now Prepared for Papers, Proposals, Physics, Presentations, Politics, Priorities, oPPortunity, People-skills, Patience and PJs. Thanks to the awesomely fantastic Palomar Transient Factory team, especially Peter Nugent, Robert Quimby, Eran Ofek and Nick Law for sharing the pains and joys of getting a factory off-the-ground. Thanks to Brad Cenko and Richard Walters for the many hours spent taming the robot on mimir2:9. Thanks to Avishay Gal-Yam and Lars Bildsten for illuminating discussions on different observational and theoretical aspects of transients in the gap. The journey from idea to first light to a factory churning out thousands of transients has been so much fun that I would not trade this experience for any other. Thanks to Marten van Kerkwijk for supporting my “fishing in new waters” project with the Canada France Hawaii Telescope. Thanks to Dale Frail for supporting a “kissing frogs” radio program. Thanks to Sterl Phinney, Linqing Wen and Samaya Nissanke for great discussions on the challenge of finding the light in the gravitational sound wave.
    [Show full text]
  • Search for Very High-Energy Gamma-Ray Emission from Pulsar-Pwn Systems with the Magic Telescope
    SUBMITTED TO THE ASTROPHYSICAL JOURNAL ON JUNE XX,2008 Preprint typeset using LATEX style emulateapj v. 10/09/06 SEARCH FOR VERY HIGH-ENERGY GAMMA-RAY EMISSION FROM PULSAR-PWN SYSTEMS WITH THE MAGIC TELESCOPE. 1 2 3 4 5 3 3 6 H. ANDERHUB ,L.A.ANTONELLI , P. ANTORANZ ,M.BACKES ,C.BAIXERAS ,S.BALESTRA ,J.A.BARRIO ,D.BASTIERI , 7 4 8 8 9 1 10 6 J. BECERRA GONZALEZ´ ,J.K.BECKER , W. BEDNAREK ,K.BERGER ,E.BERNARDINI ,A.BILAND ,R.K.BOCK , , 11 12 10 12 3 1 13 10 G. BONNOLI , P. BORDAS ,D.BORLA TRIDON , V. BOSCH-RAMON ,D.BOSE ,I.BRAUN , T.BRETZ ,D.BRITZGER , 3 10 2 10 1 3 14 7 15 M. CAMARA ,E.CARMONA ,A.CAROSI , P. COLIN ,S.COMMICHAU ,J.L.CONTRERAS ,J.CORTINA ,M.T.COSTADO , , 2 16 26 16 17 3 29 16 16 S. COVINO , F.DAZZI , ,A.DE ANGELIS , E. DE CEA DEL POZO ,R.DE LOS REYES , ,B.DE LOTTO ,M.DE MARIA , 16 7 27 18 19 1 6 13 F. DE SABATA ,C.DELGADO MENDEZ , ,A.DOM´INGUEZ ,D.DOMINIS PRESTER ,D.DORNER ,M.DORO ,D.ELSAESSER , 14 20 14 14 3 5 10 7 15 M. ERRANDO ,D.FERENC ,E.FERNANDEZ´ ,R.FIRPO ,M. V.FONSECA ,L.FONT ,N.GALANTE ,R.J.GARC´IA LOPEZ´ , , 14 7 19 10 28 5 7 15 1 M. GARCZARCZYK ,M.GAUG ,N.GODINOVIC , F.GOEBEL , ,D.HADASCH ,A.HERRERO , ,D.HILDEBRAND , 13 10 19 10 10 14 1 2 D. HOHNE¨ -MONCH¨ ,J.HOSE ,D.HRUPEC ,C.C.HSU , T.
    [Show full text]
  • The Very High Energy Characteristics of Shell-Type Snrs and Pulsar Wind Nebulae at Different Ages
    Journal of Physics: Conference Series PAPER • OPEN ACCESS Related content - Non-Thermal Photon Emission from Shell- The very high energy characteristics of shell-type Type Supernova Remnants Dou Ya-Nan and Zhang Li SNRs and Pulsar Wind Nebulae at different ages - Waveguide CO2 laser with a power per unit length of about 1 W/cm W J Witteman, M Ilieva, B I Ilyukhin et al. To cite this article: V G Sinitsyna et al 2016 J. Phys.: Conf. Ser. 718 052045 - Pulse-periodic YAG laser system with phase conjugation I Yu Anikeev, A A Gordeev, I G Zubarev et al. View the article online for updates and enhancements. This content was downloaded from IP address 131.169.5.251 on 08/02/2019 at 23:15 XIV International Conference on Topics in Astroparticle and Underground Physics (TAUP 2015) IOP Publishing Journal of Physics: Conference Series 718 (2016) 052045 doi:10.1088/1742-6596/718/5/052045 The very high energy characteristics of shell-type SNRs and Pulsar Wind Nebulae at different ages V G Sinitsyna, A Y Alaverdyan, M S Andreeva, K A Balygin, S S Borisov, I A Ivanov, A M Kirichenko, A I Klimov, I P Kozhukhova, R M Mirzafatikhov, N I Moseiko, S I Nikolsky, I E Ostashev, A I Palamarchuk,V Y Sinitsyna, I G Volokh P.N. Lebedev Physical Institute, Leninsky pr. 53, Moscow, Russia E-mail: [email protected] Abstract. The investigation of VHE gamma-ray sources by any methods, including mirror Cherenkov telescopes, touches on the problem of the cosmic ray origin and, accordingly, the role of the Galaxy in their generation.
    [Show full text]
  • Niels Lund - DTU Orbit (06/07/2017) Niels Lund
    Niels Lund - DTU Orbit (06/07/2017) Niels Lund Organisations Astrophysics 25/02/2012 → 22/07/2016 Former VIP Emeritus Associate Professor, National Space Institute 11/01/2007 → present [email protected] VIP Astrophysics and Atmospheric Physics 22/07/2016 → present VIP Publications: eXTP: enhanced X-ray Timing and Polarimetry Mission General information State: Published Organisations: National Space Institute, Astrophysics and Atmospheric Physics, Chinese Academy of Sciences, Tsinghua University, Max-Planck-Institute for Extraterrestrial Physics, Tongji University, University of Geneva Authors: Zhang, S. (Ekstern), Feroci, M. (Ekstern), Santangelo, A. (Ekstern), Dong, Y. (Ekstern), Feng, H. (Ekstern), Lu, F. (Ekstern), Nandra, K. (Ekstern), Wang, Z. (Ekstern), Zhang, S. (Ekstern), Bozzo, E. (Ekstern), Brandt, S. (Intern), Budtz- Jørgensen, C. (Intern), Lund, N. (Intern) Number of pages: 16 Publication date: 2016 Host publication information Title of host publication: Proceedings of Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray Volume: 9905 Publisher: SPIE - International Society for Optical Engineering Editors: den Herder, J. A., Takahashi, T., Bautz, M. Article number: 99051Q Main Research Area: Technical/natural sciences Conference: Space Telescopes and Instrumentation 2016, Edinburgh, United Kingdom, 26/06/2016 - 26/06/2016 X-ray astronomy, Neutron Star EOS, Strong Magnetism, Strong Gravity, X-ray timing, Spectroscopy Electronic versions: 99051Q.pdf DOIs: 10.1117/12.2232034 Bibliographical note For full list of authors, see the article: doi:10.1117/12.2232034 Publication: Research - peer-review › Article in proceedings – Annual report year: 2016 The LOFT mission concept: a status update General information State: Published Organisations: National Space Institute, Astrophysics and Atmospheric Physics, Geomagnetism Authors: Feroci, M.
    [Show full text]
  • Supernova Remnants and the Life Cycle of Interstellar Dust
    Design Reference Mission Case Study Stratospheric Observatory for Infrared Astronomy Science Steering Committee Supernova Remnants and the Life Cycle of Interstellar Dust Program contacts: Eli Dwek, Richard Arendt, Jesse Bregman, Sean Colgan, Harriet Dinerstein, Robert Gehrz, Harvey Moseley Scientific category: INTERSTELLAR MEDIUM Instruments: EXES, FLITECAM/CAM, FORCAST, FIFI-LS, HAWC, SAFIRE Hours of observation: 110 Abstract We propose to use the unique instrumental capabilities of SOFIA to conduct imaging and spectroscopic studies of supernovae (SNe), of young supernova remnants (SNRs) for which the ejecta have not yet fully mixed with the ISM, and select regions in older remnants which are interacting with the ambient ISM. These observations will address key issues within NASA’s Visions for Science quest for discovering the origin, structure, evolution and destiny of the universe: What is the origin of dust in early universe? How efficient are supernovae in producing interstellar dust? How efficient are their blast waves in destroying, processing, or even forming dust as they expand into the circumstellar and interstellar medium? How do interstellar shocks facilitate chemical reaction on the surfaces of dust grains? The answers to these questions are crucial for understanding the evolutionary cycle of interstellar dust, the role of dust in the processing of starlight and in determining the thermal balance and chemistry of the ISM, and its role in the formation of protoplanetary objects. Our proposed observations will explore crucial stages of this evolutionary cycle, most readily observed at wavelengths between ∼ 5 − 300 µm with spectral resolution from ∼ 30 − 3 × 104, and at spatial resolution of a few arcseconds, requiring therefore the unique capabilities of the different SOFIA instruments.
    [Show full text]
  • Exoplanet Secondary Atmosphere Loss and Revival Edwin S
    Exoplanet secondary atmosphere loss and revival Edwin S. Kitea,1 and Megan N. Barnetta aDepartment of the Geophysical Sciences, University of Chicago, Chicago, IL 60637 Edited by Mark Thiemens, University of California San Diego, La Jolla, CA, and approved June 19, 2020 (received for review April 3, 2020) The next step on the path toward another Earth is to find atmo- atmosphere? Or does the light (H2-dominated) and transient pri- spheres similar to those of Earth and Venus—high–molecular- mary atmosphere drag away the higher–molecular-weight species? weight (secondary) atmospheres—on rocky exoplanets. Many rocky Getting physical insight into thetransitionfromprimarytosec- exoplanets are born with thick (>10 kbar) H2-dominated atmo- ondary atmospheres is particularly important for rocky exoplanets spheres but subsequently lose their H2; this process has no known that are too hot for life. Hot rocky exoplanets are the highest signal/ Solar System analog. We study the consequences of early loss of a noise rocky targets for upcoming missions such as James Webb thick H atmosphere for subsequent occurrence of a high–molecular- 2 Space Telescope (JWST) (8) and so will be the most useful for weight atmosphere using a simple model of atmosphere evolution (including atmosphere loss to space, magma ocean crystallization, and checking our understanding of this atmospheric transition process. volcanic outgassing). We also calculate atmosphere survival for rocky Secondary atmospheres are central to the exoplanet explora- tion strategy (9, 10). Previous work on the hypothesis that pri- worlds that start with no H2.Ourresultsimplythatmostrockyexo- planets orbiting closer to their star than the habitable zone that were mary atmospheres played a role in forming secondary atmospheres formed with thick H2-dominated atmospheres lack high–molecular- includes that of Eucken in the 1940s (11), Urey (12), Cameron and weight atmospheres today.
    [Show full text]