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Articles: 2'506'133
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27 April 2024
 
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Results 1 to 10 of 10 for query "David C. Knauth". (0.00 sec.)



1.
On the Origin of the High-Ionization Intermediate-Velocity Gas Toward HD 14434
David C. Knauth; J. Christopher Howk; Kenneth R. Sembach; James T. Lauroesch; David M. Meyer;
10 Apr 2003   /  Astrophys.J. 592 (2003) 964-974
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2.
Oscillator Strengths for B-X, C-X, and E-X Transitions in Carbon Monoxide
S. R. Federman; M. Fritts; S. Cheng; K. M. Menningen; David C. Knauth; K. Fulk;
2 Dec 2000   /  Astrophys.J.Suppl. 134 (2001) 133-138
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3.
Physical Conditions in the Foreground Gas of Reflection Nebulae: NGC 2023, vdB 102, and NGC 7023
David C. Knauth; S.R. Federman; K. Pan; M. Yan; David L. Lambert;
9 Mar 2001   /  Astrophys.J.Suppl. 135 (2001) 201-226
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4.
Potential Variations in the Interstellar N I Abundance
David C. Knauth; B-G Andersson; Stephan R.McCandliss; H. Warren Moos;
14 Oct 2003   /  Astrophys.J. 596 (2003) 51-54
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5.
The Interstellar Rubidium Isotope Ratio toward Rho Ophiuchi A
S.R. Federman; David C. Knauth; David L. Lambert;
28 Dec 2003   /  Astrophys.J. 603 (2004) L105-L108
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6.
An Ultra-High-Resolution Survey of the Interstellar ^7Li-to-^6Li Isotope Ratio in the Solar Neighborhood
David C. Knauth; S. R. Federman; David L. Lambert;
10 Dec 2002   /  Astrophys.J. 586 (2003) 268-285; Erratum-ibid. 594 (2003) 664
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7.
Deuterium Toward Two Milky Way Disk Stars: Probing Extended Sight Lines with the Far Ultraviolet Spectroscopic Explorer
Charles G. Hoopes; Kenneth R. Sembach; Guillaume Hebrard; H. Warren Moos; David C. Knauth;
12 Dec 2002   /  Astrophys.J. 586 (2003) 1094-1110
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8.
Rubidium in the Interstellar Medium
Kyle M. Walker; S. R. Federman; David C. Knauth; David L. Lambert;
13 Oct 2009
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9.
The Interstellar N/O Abundance Ratio: Evidence for Local Infall?
David C. Knauth; James T. Lauroesch; David M. Meyer;
7 Jul 2006
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10.
The interstellar N2 abundance towards HD 124314 from far-ultraviolet observations
David C Knauth; B-G Andersson; Stephan R McCandliss; H Warren Moos;
10 Jun 2004   /  Nature, 429 (6992), 636-8
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