The Daily Brew
Selected astro-ph abstracts for Monday November 27
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A Possible Origin of the Mass-Metallicity Relation of Galaxies
J. Koeppen, C. Weidner and P. Kroupa
Comments: 14 pages, 19 figures; accepted for publication by MNRAS
astro-ph/0611723
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The Origin of Line Emission in Massive z~2.3 Galaxies: Evidence for
Cosmic Downsizing of AGN Host Galaxies
Mariska Kriek, Pieter G. van Dokkum, Marijn Franx, Garth D.
Illingworth, Paolo Coppi, Natascha M. Forster Schreiber, Eric Gawiser, Ivo
Labbe, Paulina Lira, Danilo Marchesini, Ryan Quadri, Gregory Rudnick, Edward
N. Taylor, C. Megan Urry and Paul P. van der Werf
Comments: Submitted to ApJ
astro-ph/0611724
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Observations of the Unidentified TeV Gamma-Ray Source TeV J2032+4130
with the Whipple Observatory 10 m Telescope
A. Konopelko, R. W. Atkins, G. Blaylock, J. H. Buckley, Y. Butt, D. A.
Carter-Lewis, O. Celik, P. Cogan, Y. C. K. Chow, W. Cui, C. Dowdall, T.
Ergin, A. D. Falcone, D. J. Fegan, S. J. Fegan, J. P. Finley, P. Fortin, G.
H. Gillanders, K. J. Gutierrez, J. Hall, D. Hanna, D. Horan, S. B. Hughes, T.
B. Humensky, A. Imran, I. Jung, P. Kaaret, G. E. Kenny, M. Kertzman, D. B.
Kieda, J. Kildea, J. Knapp, K. Kosack, H. Krawczynski, F. Krennrich, M. J.
Lang, S. LeBohec, P. Moriarty, R. Mukherjee, T. Nagai, R. A. Ong, J. S.
Perkins, M. Pohl, K. Ragan, P. T. Reynolds, H. J. Rose, G. H. Sembroski, M.
Schroedter, A. W. Smith, D. Steele, A. Syson, S. P Swordy, J. A. Toner, L.
Valcarcel, V. V. Vassiliev, R. G. Wagner, S. P. Wakely, T. C. Weekes, R. J.
White, D. A. Williams, B. Zitzer
Comments: Accepted for publication in the Astrophysical Journal
astro-ph/0611730
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TeV J2032+4130: a not-so-dark Accelerator?
Yousaf M. Butt, Jorge A. Combi, Jeremy Drake, John P. Finley,
Alexander Konopelko, Matthew Lister, Jerome Rodriguez
Comments: 17 pages, ApJL submitted
astro-ph/0611731
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AEGIS: Infrared Spectral Energy Distributions of MIPS 70micron selected
sources
M. Symeonidis (1), D. Rigopoulou (1), J.-S. Huang (2), M. Davis, M. L.
N. Ashby, P. Barmby, E. Egami, G. G. Fazio, E. LeFloc'h, G. Rieke, S. P.
Willner, G. Wilson ((1) University of Oxford, (2) Harvard University)
Comments: 4 pages, 5 figures, accepted for publication in AEGIS ApJL Special
Issue
astro-ph/0611735
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Gravitational lensing as a probe of compact object population in the
Galaxy
S. Oslowski, R. Moderski, T. Bulik, K. Belczynski
Comments: Submitted to Astronomy and Astrophysics
astro-ph/0611736
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A polarised infrared flare from Sagittarius A* and the signatures of
orbiting plasma hotspots
S. Trippe (1), T. Paumard (1), T. Ott (1), S. Gillessen (1), F.
Eisenhauer (1), F. Martins (1), R. Genzel (1 and 2) ((1) MPE Garching,
Germany (2) UC Berkeley, USA)
Comments: 9 pages, 8 figures, accepted for publication in MNRAS
astro-ph/0611737
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Evidence for a large fraction of Compton-thick quasars at high redshift
Alejo Martinez-Sansigre, Steve Rawlings, David G. Bonfield, Silvia
Mateos, Chris Simpson, Mike Watson, Omar Almaini, Sebastien Foucaud, Kazuhiro
Sekiguchi, Yoshihiro Ueda
Comments: 6 pages, 2 colour figures. Submitted to MNRAS. Full resolution
version and supplementary figures can be found at:
http://www.mpia.de/homes/martinez/publications.html
astro-ph/0611739
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Two Disk Components from a Gas Rich Disk-Disk Merger
Chris Brook, Simon Richard, Daisuke Kawata, Hugo Martel, & Brad K.
Gibson
Comments: 10 pages, 1 color figure. Accepted for publication in ApJ
astro-ph/0611748
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Cosmological neutrino mass limits: variations with choice of data sets
and a new, bias-free limit
Jostein R. Kristiansen, Oystein Elgaroy, Hakon Dahle
Comments: 7 pages, revtex4
astro-ph/0611761
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Hidden Trigger for the Giant Starburst Arc in M 83?
Ruben J. Diaz, Horacio Dottori, Maria P. Aguero, Evencio Mediavilla,
Irapuan Rodrigues, Damian Mast
Comments: 18 pages, including 4 figures (3 in color). The Astrophysical
Journal, in press
astro-ph/0611771
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ISM studies of GRB 030329 with high resolution spectroscopy
Christina C. Thoene (MPE, DARK), Jochen Greiner (MPE), Sandra Savaglio
(MPE), Emmanuel Jehin (ESO)
Comments: 11 pages, 4 figures, submitted to ApJ
astro-ph/0611772
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