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Local interstellar medium properties and deuterium abundances for the lines of sight toward HR 1099, 31 Comae, beta Ceti, and beta Cassiopeiae
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Department of Physics and Astronomy, Observational Astronomy.
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1997 (English)In: Astrophysical Journal, ISSN 0004-637X, Vol. 474, no 1, 315-328 p.Article in journal (Other scientific) Published
Abstract [en]

We analyze Goddard High-Resolution Spectrograph data to infer the properties of local interstellar gas and the deuterium/hydrogen (D/H) ratio for lines of sight toward four nearby late-type stars-HR 1099, 32 Comae, beta Ceti, and beta Cassiopeiae. The dat

Place, publisher, year, edition, pages
1997. Vol. 474, no 1, 315-328 p.
Keyword [en]
binaries; spectroscopic; ISM; abundances; ISM; clouds; ultraviolet; ISM; HIGH-RESOLUTION SPECTROGRAPH; HST-GHRS OBSERVATIONS; CANIS-MAJORIS; SOLAR-WIND; SIRIUS-A; GAS; HYDROGEN; CLOUD; CAPELLA; IONIZATION
Identifiers
URN: urn:nbn:se:uu:diva-85359OAI: oai:DiVA.org:uu-85359DiVA: diva2:113267
Note
Addresses: Piskunov N, ASTRON OBSERV, BOX 515, S-75120 UPPSALA, SWEDEN. UNIV COLORADO, JOINT INST LAB ASTROPHYS, BOULDER, CO 80309. SPACE TELESCOPE SCI INST, COMP SCI CORP, ASTRON PROGRAM, BALTIMORE, MD 21218. UNIV COLORADO, CTR ASTROPHYS & SPACE ASTRON,Available from: 2006-12-20 Created: 2006-12-20 Last updated: 2011-01-15

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