The Daily Brew
Selected astro-ph abstracts for Thursday March 29
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Where are the Cosmic Metals at z~3? Temperature distribution of the
metal-enhanced ISM/IGM, the Cosmic Metal Budget and the Cosmic Stellar IMF
Jesper Sommer-Larsen (1,2), Johan P. U. Fynbo (1) ((1) Dark Cosmology
Centre, NBI, Copenhagen; (2) Institute of Astronomy, University of Tokyo)
astro-ph/0703698
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On the Nature of Velocity Fields in High z Galaxies
Jason X. Prochaska (1), Hsiao-Wen Chen (2), Arthur M. Wolfe (3),
Miroslava Dessauges-Zavadsky (4), Joshua S. Bloom (5) ((1) UCO/Lick
Observatory, (2) U Chicago, (3) UC San Diego, (4) Observatoire de Geneve, (5)
UC Berkeley)
astro-ph/0703701
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Evidence for deuterium astration in the planetary nebula Sh2-216?
Cristina M Oliveira, Pierre Chayer, H. Warren Moos, Jeffrey W. Kruk,
Thomas Rauch
astro-ph/0703703
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ASAS Eclipsing Binaries with Observed High Period Change Rates
B. Pilecki, D. Fabrycky, R. Poleski
astro-ph/0703705
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Looking for Giant Earths in the HD 209458 System: A Search for Transits
in MOST Space-based Photometry
Bryce Croll, Jaymie M. Matthews, Jason F. Rowe, Rainer Kuschnig,
Andrew Walker, Brett Gladman, Dimitar Sasselov, Chris Cameron, Gordon A. H.
Walker, Douglas N. C. Lin, David B. Guenther, Anthony F. J. Moffat, Slavek M.
Rucinski, Werner W. Weiss
astro-ph/0703710
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Large scale structure in the HI Parkes All-Sky Survey: Filling the Voids
with HI galaxies?
S. Basilakos, M. Plionis, K. Kovac, N. Voglis
astro-ph/0703713
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Observable Signatures of a Black Hole Ejected by Gravitational Radiation
Recoil in a Galaxy Merger
Abraham Loeb (Harvard)
astro-ph/0703722
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A new method of determining the initial size and Lorentz factor of
gamma-ray burst fireballs using a thermal emission component
Asaf Pe'er, Felix Ryde, Ralph A.M.J. Wijers, Peter M\'esz\'aros and
Martin J. Rees
astro-ph/0703734
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The Opposite of Dark Energy: Limits on $w = 2/3$ Ultralight Energy in
the Early Universe
Robert J. Nemiroff
astro-ph/0703737
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Quasar H II Regions During Cosmic Reionization
Marcelo A. Alvarez and Tom Abel
astro-ph/0703740
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