Published September 19, 1979 | Version v1
Miscellaneous Open

Space distribution and physical properties of cool dwarf stars

Description

A new study of the space density of red dwarfs based on a sample of red dwarfs in a field of 238 square degrees towards the South Galactic Pole is presented. A blink survey using red and blue copies of Mount Palomar Sky Survey plates of a six square degrees field centered on the South Galactic Pole was performed and the results (approximately 2500 red objects) and the discussion of these results are presented. The time that elapsed before a black dwarf becomes invisible is estimated and is suggested that low-velocity red dwarfs could be explained by contracting black dwarfs. Based on theoretical considerations it can be shown that the existence of a large number of low-velocity stars is in serious conflict with criteria for the stability of the galactic disk. It is shown that if one also takes into account all generations of black dwarfs that are already invisible and therfore old, the mean velocity of all black dwarfs is much higher so that there is no conflict with theory. Luminosity functions of red and black dwarfs in several photometric passbands are calculated. (Auth.)

Availability note (English)

MF available from INIS under the Report Number.

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Additional details

Publishing Information

Imprint Pagination
170 p.
Report number
INIS-mf--5608

INIS

Country of Publication
Netherlands
Country of Input or Organization
Netherlands
INIS RN
11515709
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Numerical Data, Thesis
Descriptors DEI
BLACK DWARF STARS; EXPERIMENTAL DATA; GRAPHS; ISOLATED VALUES; LUMINOSITY; RED DWARF STARS; SPATIAL DISTRIBUTION; TABLES; VELOCITY
Descriptors DEC
DATA; DATA FORMS; DISTRIBUTION; DWARF STARS; INFORMATION; NUMERICAL DATA; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; STARS

Optional Information

Notes
Includes Dutch summary; includes previously published material; 120 refs.