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The luminosity function of white dwarfs and M dwarfs using dark nebulae as opaque outer screens
Uppsala University.
1998 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 336, no 3, 883-894 p.Article in journal (Other scientific) Published
Abstract [en]

By using dark nebulae as opaque outer screens, the luminosity function of white dwarfs and M dwarfs has been studied. High-extinction areas towards the Orion A, Serpens and rho Oph cloud complexes were observed, covering a volume corresponding to 464 pc(3

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1998. Vol. 336, no 3, 883-894 p.
Keyword [en]
stars : late-type; low-mass; brown dwarfs; luminosity function; mass function; white dwarfs; Galaxy : solar neighbourhood; stellar content; OPHIUCHI CLOUD CORE; STAR COUNTS; STELLAR POPULATION; GALACTIC DISK; MOLECULAR CLOUD; IMAGING SURVEY; ESO AREA-207;
Identifiers
URN: urn:nbn:se:uu:diva-85297OAI: oai:DiVA.org:uu-85297DiVA: diva2:113205
Note
Addresses: Festin L, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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