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Abstracts Connecting to the Boston University Network
20th Cambridge Workshop: Cool Stars, Stellar Systems, and the Sun July 29 - Aug 3, 2018 Boston / Cambridge, USA Abstracts Connecting to the Boston University Network 1. Select network ”BU Guest (unencrypted)” 2. Once connected, open a web browser and try to navigate to a website. You should be redirected to https://safeconnect.bu.edu:9443 for registration. If the page does not automatically redirect, go to bu.edu to be brought to the login page. 3. Enter the login information: Guest Username: CoolStars20 Password: CoolStars20 Click to accept the conditions then log in. ii Foreword Our story starts on January 31, 1980 when a small group of about 50 astronomers came to- gether, organized by Andrea Dupree, to discuss the results from the new high-energy satel- lites IUE and Einstein. Called “Cool Stars, Stellar Systems, and the Sun,” the meeting empha- sized the solar stellar connection and focused discussion on “several topics … in which the similarity is manifest: the structures of chromospheres and coronae, stellar activity, and the phenomena of mass loss,” according to the preface of the resulting, “Special Report of the Smithsonian Astrophysical Observatory.” We could easily have chosen the same topics for this meeting. Over the summer of 1980, the group met again in Bonas, France and then back in Cambridge in 1981. Nearly 40 years on, I am comfortable saying these workshops have evolved to be the premier conference series for cool star research. Cool Stars has been held largely biennially, alternating between North America and Europe. Over that time, the field of stellar astro- physics has been upended several times, first by results from Hubble, then ROSAT, then Keck and other large aperture ground-based adaptive optics telescopes. -
Calvary Lutheran Church September 2016
CALVARY LUTHERAN CHURCH SEPTEMBER 2016 Pastor Dawn L. Spies, Interim Pastor From the Pastor’s Calvary Lutheran Church Office 262.786.4010 Text 760.208.0986 INSIDE [email protected] THIS ISSUE: My wall has been covered with calendar pages! Over the summer I’ve been slowly filling it in. I started by putting on From the Pastor’s Study Cover all the dates the area school districts have off. Then I added all the annual events that we participate in here at Calvary: Thanksgiving Christian Education New Eve worship, Christmas decorating and a fun Christmas Music Event 2-3 Fall Schedule (save the date, December 4!). All the fun and fellowship is vital as we grow together in faith and friendship. High School Mission Trip 4 Our big fall kickoff went up next: Rally Day is September 18. This year, we’re going to provide some tools so we can also invite our Vacation Bible School 5 friends back to church on this weekend too! Then the Sunday School calendar – for both students and adults – was added! Having that time Women’s Ministry 6 set aside, each week, to worship, pray and study is vital! rd th Then Youth Group events for our Littlest Lutherans, 3 -5 Graders, Mission & Outreach 7 Middle School and High School were added. These were followed by events we can all participate in: like Tubing and an Epiphany Cele- bration at Luther Manor. Mallards Game Recap 8 I have a different color post-it note for each ministry. It makes me so Congregation News 9 happy!! Not just because my office planning calendar is full and col- orful, but because each post-it note represents people who eagerly de- Calendar & Serving at sire to know God and one another better. -
CONFERENCE and REVIEW PUBLICATONS, and WHITE PAPERS: Reverse Chronological Harper, GM, 2013
CONFERENCE AND REVIEW PUBLICATONS, AND WHITE PAPERS: Reverse Chronological Harper, G. M., 2013, [Invited Review] Atmospheric structure and dynamics: the spatial and temporal domains, EAS Publications Series, Vol 60, 2013, pp.59-68 Farzone, M., Ryde, N., Harper, G. M., Lambert, J., Josselin, E., Richter, M. J., & Eriksson, K., 2013, What is the Origin of the Water Vapour Signatures in Red Giant Stars?, EAS Publications Series, Vol 60, pp.155-159 Carpenter, K. G., Ayres, T., Brown, A., Harper, G. M., & Wahlgren, G. M., 2012. The Amazing COS FUV (1320 - 1460A)˚ Spectrum of λ Vel (K4Ib-II), 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. Eds. C. M. Johns-Krull, M. K. Browning, and A. A. West. San Francisco: ASP Conf Ser., Vol. 448, p.1083 Harper, G. M., Brown, A., & Redfield, S., 2012, Constraints on the Surface Magnetic Field Structure of Aldebaran (αTauri, K5 III), 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. Eds. C. M. Johns-Krull, M. K. Browning, and A. A. West. San Francisco: ASP Conf Ser., Vol. 448, p.1145 O’Gorman, E. & Harper, G. M., 2012, What is Heating Arcturus’ Wind?, 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. Eds. C. M. Johns-Krull, M. K. Browning, and A. A. West. San Francisco: ASP Conf Ser., Vol. 448, p.691 van Belle, G. T., Aufdenberg, J., Boyajian, T., Harper G. M., Hummel, C., Pedretti, E., Baines, E., White, R., Ravi, V., & Ridgway, S., 2012, Fundamental Stellar Properties from Optical Interferometry, 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. -
Publication List for Amaury H.M.J. Triaud Most Important Publications
1 Publication List for Amaury H.M.J. Triaud Listing following SAO/NASA’s ADS paper archive. There are active links to the ADS paper archive in blue. All refereed publication can be accessed by clicking here and all publications, in- cluding conference proceedings, white papers and some proposal abstracts by clicking here. LAST UPDATED ON 2015-07-16: 101 refereed publications, above 2700 citations. H-index = 30. In addition: 4 are submitted or in press, 16 are conference proceedings or white papers. Most important publications WASP-80B HAS A DAYSIDE WITHIN THE T-DWARF RANGE Triaud, Amaury H. M. J., Gillon, Michaël, Ehrenreich, David, Herrero, Enrique, Lendl, Monika, Anderson, David R., Collier Cameron, Andrew, Delrez, Laetitia, Demory, Brice-Olivier, Hellier, Coel, Heng, Kevin, Jehin, Emmanuel, Maxted, Pierre F. L., Pollacco, Don, Queloz, Didier, Ribas, Ignasi, Smalley, Barry, Smith, Alexis M. S., Udry, Stéphane 2015 MNRAS 450 2279 CIRCUMBINARY PLANETS - WHY THEY ARE SO LIKELY TO TRANSIT Martin, D. V. & Triaud, A. H. M. J. 2015 MNRAS 449, 781 PLANETS TRANSITING NON-ECLIPSING BINARIES Martin, D. V. & Triaud, A. H. M. J. 2014 A&A 570, 91 COLOUR-MAGNITUDE DIAGRAMS OF TRANSITING EXOPLANETS I-SYSTEMS WITH PARALLAXES Triaud, A. H. M. J. 2014 MNRAS 439, L61 FAST-EVOLVING WEATHER FOR THE COOLEST OF OUR TWO NEW SUBSTELLAR NEIGHBOURS Gillon, M., Triaud, A. H. M. J., Jehin, E., Delrez, L., Opitom, C., Magain, P., Lendl, M., Queloz, D. 2013 A&A 555, L5 A SEARCH FOR ROCKY PLANETS TRANSITING BROWN DWARFS Triaud, Amaury H. M. J., Gillon, Michael, Selsis, Franck, Winn, Joshua N., Demory, Brice-Olivier, Artigau, Etienne, Laughlin, Gregory P., Seager, Sara, Helling, Christiane, Mayor, Michel, Albert, Loic, Anderson, Richard I., Bolmont, Emeline, Doyon, Rene, Forveille, Thierry, Hagelberg, Janis, Leconte, Jeremy, Lendl, Monika, Littlefair, Stuart, Raymond, Sean, Sahlmann, Johannes (arXiv:1304.7248) WASP-80B: A GAS GIANT TRANSITING A COOL DWARF Triaud, A. -
2012 Annual Progress Report and 2013 Program Plan of the Gemini Observatory
2012 Annual Progress Report and 2013 Program Plan of the Gemini Observatory Association of Universities for Research in Astronomy, Inc. Table of Contents 0 Executive Summary ....................................................................................... 1 1 Introduction and Overview .............................................................................. 5 2 Science Highlights ........................................................................................... 6 2.1 Highest Resolution Optical Images of Pluto from the Ground ...................... 6 2.2 Dynamical Measurements of Extremely Massive Black Holes ...................... 6 2.3 The Best Standard Candle for Cosmology ...................................................... 7 2.4 Beginning to Solve the Cooling Flow Problem ............................................... 8 2.5 A Disappearing Dusty Disk .............................................................................. 9 2.6 Gas Morphology and Kinematics of Sub-Millimeter Galaxies........................ 9 2.7 No Intermediate-Mass Black Hole at the Center of M71 ............................... 10 3 Operations ...................................................................................................... 11 3.1 Gemini Publications and User Relationships ............................................... 11 3.2 Science Operations ........................................................................................ 12 3.2.1 ITAC Software and Queue Filling Results .................................................. -
Arxiv:0908.2624V1 [Astro-Ph.SR] 18 Aug 2009
Astronomy & Astrophysics Review manuscript No. (will be inserted by the editor) Accurate masses and radii of normal stars: Modern results and applications G. Torres · J. Andersen · A. Gim´enez Received: date / Accepted: date Abstract This paper presents and discusses a critical compilation of accurate, fun- damental determinations of stellar masses and radii. We have identified 95 detached binary systems containing 190 stars (94 eclipsing systems, and α Centauri) that satisfy our criterion that the mass and radius of both stars be known to ±3% or better. All are non-interacting systems, so the stars should have evolved as if they were single. This sample more than doubles that of the earlier similar review by Andersen (1991), extends the mass range at both ends and, for the first time, includes an extragalactic binary. In every case, we have examined the original data and recomputed the stellar parameters with a consistent set of assumptions and physical constants. To these we add interstellar reddening, effective temperature, metal abundance, rotational velocity and apsidal motion determinations when available, and we compute a number of other physical parameters, notably luminosity and distance. These accurate physical parameters reveal the effects of stellar evolution with un- precedented clarity, and we discuss the use of the data in observational tests of stellar evolution models in some detail. Earlier findings of significant structural differences between moderately fast-rotating, mildly active stars and single stars, ascribed to the presence of strong magnetic and spot activity, are confirmed beyond doubt. We also show how the best data can be used to test prescriptions for the subtle interplay be- tween convection, diffusion, and other non-classical effects in stellar models. -
GTO Keypad Manual, V5.001
ASTRO-PHYSICS GTO KEYPAD Version v5.xxx Please read the manual even if you are familiar with previous keypad versions Flash RAM Updates Keypad Java updates can be accomplished through the Internet. Check our web site www.astro-physics.com/software-updates/ November 11, 2020 ASTRO-PHYSICS KEYPAD MANUAL FOR MACH2GTO Version 5.xxx November 11, 2020 ABOUT THIS MANUAL 4 REQUIREMENTS 5 What Mount Control Box Do I Need? 5 Can I Upgrade My Present Keypad? 5 GTO KEYPAD 6 Layout and Buttons of the Keypad 6 Vacuum Fluorescent Display 6 N-S-E-W Directional Buttons 6 STOP Button 6 <PREV and NEXT> Buttons 7 Number Buttons 7 GOTO Button 7 ± Button 7 MENU / ESC Button 7 RECAL and NEXT> Buttons Pressed Simultaneously 7 ENT Button 7 Retractable Hanger 7 Keypad Protector 8 Keypad Care and Warranty 8 Warranty 8 Keypad Battery for 512K Memory Boards 8 Cleaning Red Keypad Display 8 Temperature Ratings 8 Environmental Recommendation 8 GETTING STARTED – DO THIS AT HOME, IF POSSIBLE 9 Set Up your Mount and Cable Connections 9 Gather Basic Information 9 Enter Your Location, Time and Date 9 Set Up Your Mount in the Field 10 Polar Alignment 10 Mach2GTO Daytime Alignment Routine 10 KEYPAD START UP SEQUENCE FOR NEW SETUPS OR SETUP IN NEW LOCATION 11 Assemble Your Mount 11 Startup Sequence 11 Location 11 Select Existing Location 11 Set Up New Location 11 Date and Time 12 Additional Information 12 KEYPAD START UP SEQUENCE FOR MOUNTS USED AT THE SAME LOCATION WITHOUT A COMPUTER 13 KEYPAD START UP SEQUENCE FOR COMPUTER CONTROLLED MOUNTS 14 1 OBJECTS MENU – HAVE SOME FUN! -
407 a Abell Galaxy Cluster S 373 (AGC S 373) , 351–353 Achromat
Index A Barnard 72 , 210–211 Abell Galaxy Cluster S 373 (AGC S 373) , Barnard, E.E. , 5, 389 351–353 Barnard’s loop , 5–8 Achromat , 365 Barred-ring spiral galaxy , 235 Adaptive optics (AO) , 377, 378 Barred spiral galaxy , 146, 263, 295, 345, 354 AGC S 373. See Abell Galaxy Cluster Bean Nebulae , 303–305 S 373 (AGC S 373) Bernes 145 , 132, 138, 139 Alnitak , 11 Bernes 157 , 224–226 Alpha Centauri , 129, 151 Beta Centauri , 134, 156 Angular diameter , 364 Beta Chamaeleontis , 269, 275 Antares , 129, 169, 195, 230 Beta Crucis , 137 Anteater Nebula , 184, 222–226 Beta Orionis , 18 Antennae galaxies , 114–115 Bias frames , 393, 398 Antlia , 104, 108, 116 Binning , 391, 392, 398, 404 Apochromat , 365 Black Arrow Cluster , 73, 93, 94 Apus , 240, 248 Blue Straggler Cluster , 169, 170 Aquarius , 339, 342 Bok, B. , 151 Ara , 163, 169, 181, 230 Bok Globules , 98, 216, 269 Arcminutes (arcmins) , 288, 383, 384 Box Nebula , 132, 147, 149 Arcseconds (arcsecs) , 364, 370, 371, 397 Bug Nebula , 184, 190, 192 Arditti, D. , 382 Butterfl y Cluster , 184, 204–205 Arp 245 , 105–106 Bypass (VSNR) , 34, 38, 42–44 AstroArt , 396, 406 Autoguider , 370, 371, 376, 377, 388, 389, 396 Autoguiding , 370, 376–378, 380, 388, 389 C Caldwell Catalogue , 241 Calibration frames , 392–394, 396, B 398–399 B 257 , 198 Camera cool down , 386–387 Barnard 33 , 11–14 Campbell, C.T. , 151 Barnard 47 , 195–197 Canes Venatici , 357 Barnard 51 , 195–197 Canis Major , 4, 17, 21 S. Chadwick and I. Cooper, Imaging the Southern Sky: An Amateur Astronomer’s Guide, 407 Patrick Moore’s Practical -
Annual Report / Rapport Annuel / Jahresbericht 1996
Annual Report / Rapport annuel / Jahresbericht 1996 ✦ ✦ ✦ E U R O P E A N S O U T H E R N O B S E R V A T O R Y ES O✦ 99 COVER COUVERTURE UMSCHLAG Beta Pictoris, as observed in scattered light Beta Pictoris, observée en lumière diffusée Beta Pictoris, im Streulicht bei 1,25 µm (J- at 1.25 microns (J band) with the ESO à 1,25 microns (bande J) avec le système Band) beobachtet mit dem adaptiven opti- ADONIS adaptive optics system at the 3.6-m d’optique adaptative de l’ESO, ADONIS, au schen System ADONIS am ESO-3,6-m-Tele- telescope and the Observatoire de Grenoble télescope de 3,60 m et le coronographe de skop und dem Koronographen des Obser- coronograph. l’observatoire de Grenoble. vatoriums von Grenoble. The combination of high angular resolution La combinaison de haute résolution angu- Die Kombination von hoher Winkelauflö- (0.12 arcsec) and high dynamical range laire (0,12 arcsec) et de gamme dynamique sung (0,12 Bogensekunden) und hohem dy- (105) allows to image the disk to only 24 AU élevée (105) permet de reproduire le disque namischen Bereich (105) erlaubt es, die from the star. Inside 50 AU, the main plane jusqu’à seulement 24 UA de l’étoile. A Scheibe bis zu einem Abstand von nur 24 AE of the disk is inclined with respect to the l’intérieur de 50 UA, le plan principal du vom Stern abzubilden. Innerhalb von 50 AE outer part. Observers: J.-L. Beuzit, A.-M. -
Arxiv:2006.10868V2 [Astro-Ph.SR] 9 Apr 2021 Spain and Institut D’Estudis Espacials De Catalunya (IEEC), C/Gran Capit`A2-4, E-08034 2 Serenelli, Weiss, Aerts Et Al
Noname manuscript No. (will be inserted by the editor) Weighing stars from birth to death: mass determination methods across the HRD Aldo Serenelli · Achim Weiss · Conny Aerts · George C. Angelou · David Baroch · Nate Bastian · Paul G. Beck · Maria Bergemann · Joachim M. Bestenlehner · Ian Czekala · Nancy Elias-Rosa · Ana Escorza · Vincent Van Eylen · Diane K. Feuillet · Davide Gandolfi · Mark Gieles · L´eoGirardi · Yveline Lebreton · Nicolas Lodieu · Marie Martig · Marcelo M. Miller Bertolami · Joey S.G. Mombarg · Juan Carlos Morales · Andr´esMoya · Benard Nsamba · KreˇsimirPavlovski · May G. Pedersen · Ignasi Ribas · Fabian R.N. Schneider · Victor Silva Aguirre · Keivan G. Stassun · Eline Tolstoy · Pier-Emmanuel Tremblay · Konstanze Zwintz Received: date / Accepted: date A. Serenelli Institute of Space Sciences (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E- 08193, Spain and Institut d'Estudis Espacials de Catalunya (IEEC), Carrer Gran Capita 2, Barcelona, E-08034, Spain E-mail: [email protected] A. Weiss Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany C. Aerts Institute of Astronomy, Department of Physics & Astronomy, KU Leuven, Celestijnenlaan 200 D, 3001 Leuven, Belgium and Department of Astrophysics, IMAPP, Radboud University Nijmegen, Heyendaalseweg 135, 6525 AJ Nijmegen, the Netherlands G.C. Angelou Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany D. Baroch J. C. Morales I. Ribas Institute of· Space Sciences· (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E-08193, arXiv:2006.10868v2 [astro-ph.SR] 9 Apr 2021 Spain and Institut d'Estudis Espacials de Catalunya (IEEC), C/Gran Capit`a2-4, E-08034 2 Serenelli, Weiss, Aerts et al. -
6<10 JULY 2015
()!""#$*+%&* ,$'&()*( *+!,"'-,.#//,0,+12+,.#//,)'%%!)*1'% #,34567849,:4;<7=>?,4>,@8A,54BA,4:,CD77,B477,=>,@8A,BD@A, 7@D?A7,4:,7@ABBD5,AE4B<@=4>,4:,7@D57,4:,DBB,CD77A7 (62*$5&+,1* ;<=>*?@AB*C>=D -.'$/%&$*(0.12''2"#*34%562#4 !"#"$%&'(")*+,"! 6FLHQWLƄF2UJDQLVLQJ&RPPLWWHH 7#82$45*(94%:4/'*7#&6054 -../"0.1'/"234"-.56./7"8.(9'5:; -HDQ3KLOOLSH%HUJHUs+HQUL%RIĺQ <5=>//."[email protected]/.&"24B"4%%=>(>7"<C.D./; U>(./M'/"85W>&&>L>("X"J&>F>:"?>&%.& -'E"?5:%F&.G="2H<I7"J.&:>/G; <5=>//."[email protected]/.&"X"K@L.&M>"?5:%F&.G= K@L.&M>"?5:%F&.G="24B"N'//.=@M>7"4<$; S@.("3>=M/.&"X"P&>/E"3.&=1FL>5: H&'1"->9>D.1"2IO$7"P&>/1.; $9/.="-.L&."X"I&=@(>"D."N>&1@ Q>@(>"N>&'9@"24B"Q>D@6>7"RM>(G; N'V>V@"N>M=55&>"X"R>'/"N10@/>(D S@F/"N@//'.&"24B"N'1F'9>/7"4<$; J.@&9.="N.G/.M"X"8./@'M"N@==.& $/'M>"K'1F>&D="2S8O$7"4B"N>/1F.=M.&7"43; ?>/="I(@A==@/"X"O(>5D'>"Q>(>D'/' T@5M.&"U(.::'/9="2OF>(:.&=7"<C.D./; 6RĺD5DPVWHGWs$QLWD5LFKDUGV S.&.:G"T>(=F"2H<I7"J.&:>/G; ->5&./1."<>L'/"X"Y>MF>/"<:'MF N>&V5="T'MMV@C=V'"2H<I7"J.&:>/G; -.@/>&D@"Z.=M'"X"$(L.&M"['W(=M&> /RFDO2UJDQLVLQJ&RPPLWWHH <M.((>"OF>='@M'=\3('/9/.&"X"S>=@/"J&5/F5M -'E"?5:%F&.G="X"3>M."N>95'&. S.&.:G"T>(=F"X"N>&V5="T'MMV@C=V' !"#$%&$' !"#$!%#!&'&() *""$+,,---'#!&'&(),!./,0##"/1)! ,2345,678962345'*"0: ! ! STELLAR END PRODUCTS – THE LOW MASS – HIGH MASS CONNECTION ! 6-10 July, 2015 in Garching, Germany Programme Overview 13:00 Registration 14:00 Tim De Zeeuw Welcome and Opening 14:10 SOC/LOC Announcements Session 1: Overview (Chair: Liz Humphreys) 14:20 Albert Zijlstra (invited) Grand Overview 15:00 Eric Lagadec Summary of the Recent Physics -
Epilogue: Final Salute to a Hero
Epilogue: Final salute to a hero Prior to leaving NASA, Wally Schirra narrated a 12-inch album about the Apollo 11 mis- sion called Flight to the Moon , which was released after his retirement. The fi rst side was called Moments in Space History and detailed all of NASA’s manned space missions up to the fi rst lunar landing, while the reverse side had as its title The Actual Voyage of Apollo 11 . “That’s what gave me enough money after taxes to buy that Maserati downstairs,” he told one reporter with a chuckle in his voice. In 1967, he was offered a position as a director with Imperial American (Oil and Gas) by oil tycoon John M. King , who owned more airplanes than most small airplane compa- nies. A fl amboyant Colorado millionaire entrepreneur, King was a large man given to wearing cowboy hats and boots, who was once described as having built his empire on the sound American business principle of tax avoidance through oil leasing and other per- fectly legal means. “I gave King a ride once in a T-38,” Schirra recalled with a smile. “Not legal, of course, but this sort of thing is now past the statute of limitations. We buzzed King’s ranch in Colorado, and blew the windows out!” Although Schirra worked for King in Colorado, he did not fl y any of the airplanes in the fl eet. “At fi rst I tried to fl y,” he said. “King had enough airplanes to keep me busy – a Jetstar, Electra, Lears, twin Navions with rocket assist – but fl ying and talking to clients didn’t mix.