The Daily Brew
Selected astro-ph abstracts for Tuesday February 3
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Morphological Type Dependence in the Tully-Fisher Relationship
David G. Russell
astro-ph/0402001
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Beating Lensing Cosmic Variance with Galaxy Tomography
Ue-Li Pen
astro-ph/0402008
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A Masing Molecular Cloud in the Central Parsecs of Mrk348
A.B. Peck (1), C. Henkel (2), and J.S. Ulvestad (3) ((1) Harvard
Smithsonian CfA, (2) MPIfR Bonn, (3) NRAO)
astro-ph/0402018
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The Environmental Dependence of the Relations between Stellar Mass,
Structure, Star Formation and Nuclear Activity in Galaxies
Guinevere Kauffmann, Simon D.M. White, Timothy M. Heckman, Brice
Menard, Jarle Brinchmann, Stephane Charlot, Christy Tremonti, Jon Brinkmann
astro-ph/0402030
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On the discovery of an enormous ionized halo around the hot DO white
dwarf PG1034+001
Thomas Rauch (1 and 2), Florian Kerber (3) and Eva-Maria Pauli (1)
((1) Dr.-Remeis-Sternwarte, Bamberg, Germany, (2) Institut fuer Astronomie
und Astrophysik, Tuebingen, Germany, (3) ST-ECF, Garching, Germany)
astro-ph/0402036
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Gravoturbulent Fragmentation
Ralf S. Klessen (1) & Javier Ballesteros-Paredes (2), (1 =
Astrophysical Institute Potsdam, 2=Centro de Radioastronomia y Astrofisica,
UNAM)
astro-ph/0402038
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Chemical abundances in quasar host galaxies and environments from narrow
absorption line systems
Valentina D'Odorico (1), Stefano Cristiani (2), Donatella Romano (3),
Gian Luigi Granato (4) e Luigi Danese (1) ((1) SISSA - Trieste, (2) INAF -
Trieste, (3) INAF - Bologna, (4) INAF - Padova)
astro-ph/0402043
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Semi-analytic Simulations of Galactic Winds: Volume Filling Factor,
Ejection of Metals and Parameter Study
Serena Bertone (1,2), Felix Stoehr (1,3) and Simon D. M. White (1)
((1) MPA Garching, (2) Universita' di Torino, (3) IAP Paris)
astro-ph/0402044
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Testing White Dwarf Crystallization Theory with Asteroseismology of the
Massive Pulsating DA Star BPM 37093
T.S. Metcalfe, M.H. Montgomery, A. Kanaan
astro-ph/0402046
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The metallicity-luminosity relation at medium redshift based on faint
CADIS emission line galaxies
C. Maier (1,2), K. Meisenheimer (1), H. Hippelein (1), ((1) MPIA
Heidelberg Germany, (2) ETH Hoenggerberg Zuerich)
astro-ph/0402048
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