The Daily Brew
Selected astro-ph abstracts for Wednesday 2013 February 27
- Using High-Resolution Optical Spectra to Measure Intrinsic Properties of Low-Mass Stars: New Properties for KOI-314 and GJ 3470.
J. Sebastian Pineda, Michael Bottom, John A. Johnson
arXiv:1302.6231v1
- Herschel/HIFI search for H2-17O and H2-18O in IRC+10216: constraints on models for the origin of water vapor.
David A. Neufeld (JHU), Volker Tolls (CfA), Marcelino Agúndez (Bordeaux), Eduardo González-Alfonso (Alcalá de Henares), Leen Decin (KU Leuven & Amsterdam), Fabien Daniel (CAB), José Cernicharo (CAB), Gary J. Melnick (CfA), Miroslaw Schmidt (N. Copernicus), Ryszard Szczerba (N. Copernicus)
arXiv:1302.6233v1
- A redline starburst: CO(2-1) observations of an Eddington-limited galaxy reveal star formation at its most extreme.
J. E. Geach (McGill), R. C. Hickox (Dartmouth), A. M. Diamond-Stanic (UCSD), M. Krips (IRAM), J. Moustakas (Siena College), C. A. Tremonti (Wisconsin-Madison), A. L. Coil (UCSD), P. H. Sell (Wisconsin-Madison), G. H. Rudnick (Kansas)
arXiv:1302.6236v1
- The strong environmental dependence of black hole scaling relations.
Sean L. McGee (Leiden)
arXiv:1302.6237v1
- On The Robustness of z=0-1 Galaxy Size Measurements Through Model and Non-Parametric Fits.
Moein Mosleh, Rik J. Williams, Marijn Franx
arXiv:1302.6240v1
- Giant planets orbiting metal-rich stars show signatures of planet-planet interactions.
Rebekah I. Dawson, Ruth A. Murray-Clay
arXiv:1302.6244v1
- The Cluster and Field Galaxy AGN Fraction at z = 1 to 1.5: Evidence for a Reversal of the Local Anticorrelation Between Environment and AGN Fraction.
Paul Martini (The Ohio State University), Eric D. Miller, M. Brodwin, S.A. Stanford, Anthony H. Gonzalez, M. Bautz, R.C. Hickox, D. Stern, P.R. Eisenhardt, A. Galametz, D. Norman, B.T. Jannuzi, A. Dey, S. Murray, C. Jones, M.J.I. Brown
arXiv:1302.6253v1
- First Search for Dark Matter Annihilation in the Sun Using the ANTARES Neutrino Telescope.
ANTARES Collaboration : S. Adrián-Martinez, I. Al Samarai, A. Albert, M. André, M. Anghinolfi, G. Anton, L. Anton, S. Anvar, M. Ardid, T. Astraatmadjaote, J-J. Aubert, B. Baret, S. Basa, V. Bertin, S. Biagi, C. Bigongiari, C. Bogazzi, B. Bouhou, M.C. Bouwhuis, J.Brünner, J. Busto, A. Capone, C. Cârloganu, J. Carr, S. Cecchini, Z. Charif, Ph. Charvis, T. Chiarusi, M. Circella, F. Classen, R. Coniglione, L. Core, H. Costantini, P. Coyle, A. Creusot, C. Curtil, G. De Bonis, M.P. Decowski, I. Dekeyser, A. Deschamps, C. Distefano, C. Donzaud, D. Dornic, Q. Dorosti, D. Drouhin, A. Dumas, T. Eberl, U. Emanuele, A. Enzenhöfer, J-P. Ernenwein, S. Escoffier, K. Fehn, P. Fermani, S. Ferry, V. Flaminio, F. Folger, U. Fritsch, J-L. Fuda, S. Galatà, P. Gay, S. Geisselsöder,et al. (94 additional authors not shown)
arXiv:1302.6516v1
- Explaining the Sr and Ba Scatter in Extremely Metal-Poor Stars.
Wako Aoki, Takuma Suda, Richard Boyd, Toshitaka Kajino, Michael Famiano
arXiv:1302.6573v1
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