The Daily Brew
Selected astro-ph abstracts for Wednesday February 23
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Spectroscopic Identification of a Proto-Cluster at z=2.300:
Environmental Dependence of Galaxy Properties at High Redshift
Charles C. Steidel (Caltech), Kurt L. Adelberger (OCIW), Alice E.
Shapley (UC Berkeley), Dawn K. Erb (Caltech), Naveen A. Reddy (Caltech) and
Max Pettini (IoA)
astro-ph/0502432
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Variability of Fe II Emission Features in the Seyfert 1 Galaxy NGC 5548
M. Vestergaard (1,2) and B. M. Peterson (2) ((1) Steward Observatory,
University of Arizona, (2) The Ohio State University)
astro-ph/0502433
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Finite Source Effects in Strong Lensing: Implications for the
Substructure Mass Scale
Gregory Dobler & Charles R. Keeton
astro-ph/0502436
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Red variables in the OGLE-II data base -- III. Constraints on the
three-dimensional structures of the LMC and SMC
P. Lah, L.L. Kiss, T.R. Bedding
astro-ph/0502440
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Evidence for Planet-Planet Scattering in Upsilon Andromedae
Eric B. Ford (1), Verene Lystad (2), Frederic A. Rasio (2) ((1)
University of California Berkeley, (2) Northwestern University)
astro-ph/0502441
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Panoramic Views of Cluster-Scale Assembly Explored by Subaru Wide-Field
Imaging
Tadayuki Kodama (National Astronomical Observatory of Japan) and the
PISCES team
astro-ph/0502444
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On the origin of the radial mass density profile of the Galactic halo
Globular Cluster System
Genevieve Parmentier (1), Eva K. Grebel (2) ((1) IoA, Cambridge, UK -
(2) Astronomical Institute, University of Basel, Switzerland)
astro-ph/0502447
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High Energy Neutrinos from the TeV Blazar 1ES 1959+650
Francis Halzen and Dan Hooper
astro-ph/0502449
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Cooling and Clusters: When Is Heating Needed?
Greg L. Bryan, G. Mark Voit
astro-ph/0502458
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Mixed Morphology Pairs as a Breeding Ground for Active Nuclei
Donovan L. Domingue, Jack W. Sulentic, Adriana Durbala
astro-ph/0502459
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Evidence for an Untruncated Accretion Disk in the Broad-Line Radio
Galaxy 4C+74.26
D.R. Ballantyne (1), A.C. Fabian (2) ((1) CITA, Toronto (2) IoA,
Cambridge)
astro-ph/0502461
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Do observations prove that cosmological neutrinos are thermally
distributed?
A. Cuoco, J. Lesgourgues, G. Mangano, S. Pastor
astro-ph/0502465
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