The Daily Brew
Selected astro-ph abstracts for Monday February 10
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Parallel Universes
Max Tegmark (Penn)
astro-ph/0302131
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The Araucaria Project: Dependence of mean K, J, and I absolute
magnitudes of red clump stars on metallicity and age
G. Pietrzy{\'n}ski, W. Gieren, A. Udalski
astro-ph/0302134
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The Early Light Curve of the Optical Afterglow of GRB 021211
Weidong Li, Alexei V. Filippenko, Ryan Chornock, and Saurabh Jha
(University of California, Berkeley)
astro-ph/0302136
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Imaging Large Scale Structure in the X-ray Sky
Y. Yang (UMD, LHEA/GSFC), R. F. Mushotzky (LHEA/GSFC), A. J. Barger
(U.Wisc, U.Hawaii, Ifa), L. L. Cowie (IfA), D. B. Sanders (IfA, Mpe), A. T.
Steffen (U.Wisc)
astro-ph/0302137
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The correlation of the Lyman-alpha forest in close pairs and groups of
high-redshift quasars: clustering of matter on scales 1-5 Mpc
E. Rollinde (IAP), P. Petitjean (IAP), C. Pichon (Obs. Strasbourg), S.
Colombi (IAP), B. Aracil (IAP), V. D'Odorico (IAP), M.G. Haehnelt (IoA)
astro-ph/0302145
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The Absorption and Emission Kinematics in the z=0.7450 Mg II Absorber
Towards Q1331+17
Sara L. Ellison, Gabriela Mallen-Ornelas, Marcin Sawicki
astro-ph/0302147
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Fe K emission and absorption features in XMM-Newton spectra of Mkn 766 -
evidence for reprocessing in flare ejecta
K.A. Pounds (1), J.N. Reeves (1,2), K.L. Page (1), G.A. Wynn (1), P.T.
O'Brien (1) ((1) University of Leicester, (2) Lab. for High Energy
Astrophysics, NASA GSFC)
astro-ph/0302151
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CO emission and associated HI absorption from a massive gas reservoir
surrounding the z=3 radio galaxy B3 J2330+3927
Carlos De Breuck (IAP), Roberto Neri (IRAM), Raffaella Morganti
(ASTRON), Alain Omont (IAP), Brigitte Rocca-Volmerange (IAP), Daniel Stern
(JPL), Michiel Reuland (IGPP/LLNL), Wil van Breugel (IGPP/LLNL), Huub
Rottgering (Leiden), S. A. Stanford (IGPP/LLNL and UC Davis), Hyron Spinrad
(UCB), Mario Vigotti (RAL Bologna), and Melvyn Wright (RAL, UCB)
astro-ph/0302154
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Spectral Energy Distributions of Dusty Galaxies
Toshinobu Takagi, Vladas Vansevicius, Nobuo Arimoto
astro-ph/0302157
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