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The luminosity function of main-sequence stars within 80 parsecs from Hipparcos data

Abstract:
The basic data discussed here consist of parallaxes and apparent magnitudes of more than 6000 stars with delta < -26 degrees from the Hipparcos Catalogue which were selected from the Michigan Spectral Catalogue to have estimated spectroscopic distances within 80 parsecs. The statistical properties of the sample are briefly discussed, and the luminosity function of main sequence stars is determined by the maximum-volume method from nearly 3000 stars with observed parallaxes greater than 12.5 mas.
Publication status:
Published

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Role:
Author


Journal:
HIPPARCOS VENICE '97 More from this journal
Volume:
402
Pages:
485-488
Publication date:
1997-01-01
Event title:
Hipparcos Venice 97
ISSN:
0379-6566
ISBN:
9290922915


Keywords:
Pubs id:
pubs:29110
UUID:
uuid:9c12d634-3fc1-4872-ba8e-d5372e558b83
Local pid:
pubs:29110
Source identifiers:
29110
Deposit date:
2012-12-19

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