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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 1997 (English)In: Astrophysical Journal, ISSN 0004-637X, Vol. 474, no 1, p. 315-328Article 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, p. 315-328

Keywords [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, id: 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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Piskunov, Nikolai

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Department of Astronomy and Space PhysicsObservational Astrophysics

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