Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2020-06-22T13:14:13Z
dc.date.available 2020-06-22T13:14:13Z
dc.date.issued 1973
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/98698
dc.description.abstract The distribution of the mass function of bright spectroscopic binaries is studied for systems with dwarf and with giant primaries. It is found that the distribution is very similar in both cases. Assuming that the inclination has a random distribution and postulating different distribution functions for the mass ratio, it is found that the distribution of the mass function depends only weakly upon the distribution function of the mass ratio. Apparently a distribution law f f(μ) = μ^(-7/3) reproduces well the observed statistics, provided that μ varies between 1 and 0.25. These results are in agreement with those found by C. Jaschek in Publ. Obs. Geneve, N* 24 (1971). The paper in full will be published elsewhere. en
dc.language es es
dc.subject Galaxias es
dc.title The mass function in spectroscopic binaries en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Jaschek, Carlos es
sedici.creator.person Ferrer, Osvaldo Eduardo es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 17 es


Descargar archivos

Thumbnail
Resumen (1 p.)
Descargar archivo (146.3Kb) - PDF

Este ítem aparece en la(s) siguiente(s) colección(ones)

Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)