The Daily Brew
Selected astro-ph abstracts for Tuesday 2010 June 15
- Accurate Coordinates and 2MASS Cross-IDs for (Almost) All Gliese Catalog Stars.
John Stauffer (1), Angelle M. Tanner (2), Geoffrey Bryden (3,4), Solange Ramirez (3), Bruce Berriman (3), David R. Ciardi (3), Stephen Kane (3), Trisha Mizusawa (3), Alan Payne (5), Peter Plavchan (3), Kaspar von Braun (3), Pamela Wyatt (3), J. Davy Kirkpatrick (6) ((1)Spitzer Science Center, (2)Georgia State University, (3)NExScI, (4)JPL, (5)Australian National University,(6)IPAC)
arXiv:1006.2441v1
- Particle acceleration in the expanding blast wave of Eta Carina ' s Great Eruption of 1843.
S. Ohm, J.A. Hinton, W. Domainko
arXiv:1006.2464v1
- Deep Near-Infrared Imaging of the rho Oph Cloud Core: Clues to the Origin of the Lowest-Mass Brown Dwarfs.
Kenneth A. Marsh, Peter Plavchan, J. Davy Kirkpatrick, Patrick J. Lowrance, Roc M. Cutri, Thangasamy Velusamy
arXiv:1006.2506v1
- WASP-21b: a hot-Saturn exoplanet transiting a thick disc star.
F. Bouchy, L. Hebb, I. Skillen, A. Collier Cameron, B. Smalley, S. Udry, D.R. Anderson, I. Boisse, B. Enoch, C.A. Haswell, G. Hébrard, C. Hellier, Y. Joshi, S.R. Kane, P.F.L. Maxted, M. Mayor, C. Moutou, F. Pepe, D. Pollacco, D. Queloz, D. Ségransan, E.K. Simpson, A.M.S. Smith, H.C. Stempels, R. Street, A.H.M.J. Triaud, R.G. West, P.J. Wheatley
arXiv:1006.2605v1
- Towards an explanation for the 30 Dor (LMC) Honeycomb nebula - the impact of recent observations and spectral analysis.
John Meaburn (1), Matt P. Redman (2), Panos Boumis (3), Eamonn Harvey (2) ((1) Jodrell Bank Centre for Astrophysics, University of Manchester, UK, (2) Centre for Astronomy, School of Physics, National University of Ireland Galway, Ireland (3) Institute of Astronomy & Astrophysics, National Observatory of Athens, Greece)
arXiv:1006.2692v1
- Five Kepler target stars that show multiple transiting exoplanet candidates.
Jason H. Steffen (1), Natalie M. Batalha (2), William J. Borucki (3), Lars A. Buchhave (4,5), Douglas A. Caldwell (3,10), William D. Cochran (6), Michael Endl (6), Daniel C. Fabrycky (4), François Fressin (4), Eric B. Ford (7), Jonathan J. Fortney (8), Michael J. Haas (3), Matthew J. Holman (4), Howard Isaacson (9), Jon M. Jenkins (3,10), David Koch (3), David W. Latham (4), Jack J. Lissauer (3), Althea V. Moorhead (7), Robert C. Morehead (7), Geoffrey Marcy (9), Phillip J. MacQueen (6), Samuel N. Quinn (4), Darin Ragozzine (4), Jason F. Rowe (3), Dimitar D. Sasselov (4) Sara Seager (11) Guillermo Torres (4), William F. Welsh (12), ((1) Fermilab Center for Particle Astrophysics, P.O. Box 500, Batavia, IL 60510, (2) Department of Astronomy and Physics, San Jose State University, San Jose, CA 95192, (3) NASA Ames Research Center, Moffett Field, CA 94035, (4) Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, (5) Niels Bohr Institute, Copenhagen University, DK-2100 Copenhagen, Denmark, (6) McDonald Observatory, The University of Texas, Austin, TX 78712-2059 USA, (7) Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611-2055, USA, (8) Department of Astronomy and Astrophysics, Unvirsity of California, Santa Cruz, 95064, (9) Astronomy Department, UC Berkeley, Berkeley, CA 94720, (10) SETI Institute, 515 North Whisman Road, Mountain View, CA, 94043, (11) Department of Physics, Massachussets Institute of Technology, (12) San Diego State University, 5500 Campanile Drive, San Diego, CA 92182)
arXiv:1006.2763v1
- Characteristics of Kepler Planetary Candidates Based on the First Data Set: The Majority are Found to be Neptune-Size and Smaller.
William J. Borucki,for the Kepler Team
arXiv:1006.2799v1
- Kepler Eclipsing Binary Stars. I. Catalog and Principal Characterization of 1832 Eclipsing Binaries in the First Data Release.
Andrej Prsa, Natalie M. Batalha, Robert W. Slawson, Laurance R. Doyle, William F. Welsh, Jerome A. Orosz, Sara Seager, Michael Rucker, Kimberly Mjaseth, Scott G. Engle, Kyle Conroy, Jon M. Jenkins, Douglas A. Caldwell, David G. Koch, William J. Borucki
arXiv:1006.2815v1
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