activity
19992018
most citedInterstellar Carbon in Translucent Sightlines

246 citations · 2.4k across the 44 of their papers we have counts for

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Showing 2006Show all

8 papers · 1 filter

astro-ph2006★ 52 cited

A Cold Nearby Cloud Inside the Local Bubble

David M. Meyer, J. T. Lauroesch, Carl Heiles +2

The high-latitude Galactic H I cloud toward the extragalactic radio source 3C 225 is characterized by very narrow 21 cm emission and absorption indicative of a very low H I spin te…

astro-ph2006★ 52 cited

The nature of damped Lyman alpha and sub-damped Lyman alpha absorbers

Pushpa Khare, Varsha P. Kulkarni, Celine Peroux +3

We present arguments based on the measured abundances in individual damped Lyman alpha systems (DLAs) and sub-damped Lyman alpha systems (sub-DLAs), and also the average abundances…

astro-ph2006★ 77 cited

The Role of Sub-damped Lyman-alpha Absorbers in the Cosmic Evolution of Metals

V. P. Kulkarni, P. Khare, C. Peroux +3

Observations of low mean metallicity of damped Lyman-alpha (DLA) quasar absorbers at all redshifts studied appear to contradict the predictions for the global mean interstellar met…

astro-ph2006★ 58 cited

Metal-rich Damped/sub-Damped Lyman-alpha Quasar Absorbers at z<1

C. Peroux, J. D. Meiring, V. P. Kulkarni +5

Damped Lyman-alpha absorbers (DLAs), seen in absorption against a background quasar, provide the most detailed probes available of element abundances in the Universe over > 90 % of…

astro-ph2006★ 26 cited

The Interstellar N/O Abundance Ratio: Evidence for Local Infall?

David C. Knauth, James T. Lauroesch, David M. Meyer

Sensitive measurements of the interstellar gas-phase oxygen abundance have revealed a slight oxygen deficiency ( 15%) toward stars within 500 pc of the Sun as compared to mor…

astro-ph2006★ 54 cited

Elemental Abundance Measurements in Low-redshift Damped Lyman Alpha Absorbers

Joseph D. Meiring, Varsha P. Kulkarni, Pushpa Khare +6

We present elemental abundance measurements for 9 damped Ly-alpha systems (DLAs) and 1 sub-DLA at 0.1 < z < 1.5 from recent observations with the Multiple Mirror Telescope. Most of…