The Daily Brew
Selected astro-ph abstracts for Tuesday June 17
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High-Resolution Spectroscopy of Gamma-Ray Lines from the X-Class Solar
Flare of 23 July, 2002
David M. Smith, Gerald H. Share, Ronald J. Murphy, Richard A.
Schwartz, Albert Y. Shih, and Robert P. Lin
astro-ph/0306292
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Lithium in the Symbiotic Mira V407 Cyg
A.A. Tatarnikova (1), P.M. Marrese (2), U. Munari (2), T. Tomov (3),
P. A. Whitelock (4), B.F. Yudin (1). ((1) Sternberg Astronomical Institute,
Russia; (2) INAF-Osservatorio Astronomico di Padova, Italy; (3) Centre for
Astronomy, Nicholaus Copernicus University, Poland; (4) South African
Astronomical Observatory, South Africa)
astro-ph/0306295
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Evidence for Supernova Signatures in the Spectrum of the Late-time Bump
of the Optical Afterglow of GRB 021211
M. Della Valle, D. Malesani, S. Benetti, V. Testa, M. Hamuy, L.A.
Antonelli, G. Chincarini, G. Cocozza, S. Covino, P. D'Avanzo, D. Fugazza, G.
Ghisellini, R. Gilmozzi, D. Lazzati, E. Mason, P. Mazzali, L. Stella
astro-ph/0306298
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The Munich Near-Infrared Cluster Survey (MUNICS) -- II. The K-Band
Luminosity Function of Field Galaxies to z ~ 1.2
N. Drory (1), R. Bender (2,3), G. Feulner (3), U. Hopp (3), C.
Maraston (2), J. Snigula (3), and G. J. Hill (1) ((1) University of Texas at
Austin, (2) Max-Planck-Institut fuer extraterrestrische Physik, Garching, (3)
Universitaets-Sternwarte Muenchen)
astro-ph/0306299
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Cluster AgeS Experiment (CASE): RR Lyrae stars from the globular cluster
Omega Centauri as standard candles
A. Olech, J. Kaluzny, I.B. Thompson and A. Schwarzenberg-Czerny
astro-ph/0306303
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Constraining slow-roll inflation with WMAP and 2dF
Samuel M Leach and Andrew R Liddle
astro-ph/0306305
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Are stellar coronae optically thin in X-rays? - A systematic
investigation of opacity effects
J.-U. Ness, J.H.M.M. Schmitt, M. Audard, M. Guedel, R. Mewe
astro-ph/0306308
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Decay Properties of K-Vacancy States in Fe X-Fe XVII
C. Mendoza, M.A. Bautista, T.R. Kallman, P. Palmeri
astro-ph/0306320
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Modeling of iron K lines: radiative and Auger decay data for Fe II-Fe IX
P. Palmeri, C. Mendoza, T.R. Kallman, M.A. Bautista, M. Melendez
astro-ph/0306321
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