[TTW2011] SDSS J1435+3604 68-12 , the SIMBAD biblio

[TTW2011] SDSS J1435+3604 68-12 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST06:34:18


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Title First 3 Authors
2011ApJ...732...35M 2 15 67 The first observations of low-redshift damped Lyα systems with the cosmic origins spectrograph. MEIRING J.D., TRIPP T.M., PROCHASKA J.X., et al.
2011Sci...334..948T 2 75 439 The large, oxygen-rich halos of star-forming galaxies are a major reservoir of Galactic metals. TUMLINSON J., THOM C., WERK J.K., et al.
2012ApJS..198....3W 100 82 The COS-Halos survey: Keck LRIS and Magellan MagE optical spectroscopy. WERK J.K., PROCHASKA J.X., THOM C., et al.
2012ApJ...744...93B 1 18 46 The first observations of low-redshift damped Lyα systems with the cosmic origins spectrograph: chemical abundances and affiliated galaxies. BATTISTI A.J., MEIRING J.D., TRIPP T.M., et al.
2013ApJS..204...17W 1 75 279 The COS-halos survey: an empirical description of metal-line absorption in the low-redshift circumgalactic medium. WERK J.K., PROCHASKA J.X., THOM C., et al.
2014ApJ...784..142S 79 51 Where do galaxies end? SHULL J.M.
2014ApJ...792....8W 5 44 479 The COS-halos survey: physical conditions and baryonic mass in the low-redshift circumgalactic medium. WERK J.K., PROCHASKA J.X., TUMLINSON J., et al.
2015MNRAS.449.3263J viz 16       D               1 154 124 On the possible environmental effect in distributing heavy elements beyond individual gaseous haloes. JOHNSON S.D., CHEN H.-W. and MULCHAEY J.S.
2018ApJ...865...91S 16       D               1 32 25 Does circumgalactic O VI trace low-pressure gas beyond the accretion shock? Clues from H I and low-ion absorption, line kinematics, and dust extinction. STERN J., FAUCHER-GIGUERE C.-A., HENNAWI J.F., et al.
2019MNRAS.488.2549S 48           X         1 8 58 Cooling flow solutions for the circumgalactic medium. STERN J., FIELDING D., FAUCHER-GIGUERE C.-A., et al.
2020ApJ...890...33B 16       D               1 32 ~ Interpreting observations of absorption lines in the circumgalactic medium with a turbulent medium. BUIE II E., FUMAGALLI M. and SCANNAPIECO E.
2021MNRAS.501.5575A 100       D         F     2 42 17 Most of the cool CGM of star-forming galaxies is not produced by supernova feedback. AFRUNI A., FRATERNALI F. and PEZZULLI G.
2023ApJ...956...92F 17       D               1 27 ~ The Cool Circumgalactic Medium of Low-redshift Star-forming Galaxies. I. Empirical Model and Mean Properties. FAERMAN Y. and WERK J.K.

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