The binary system AM Herculis and the parameters of its components

Details The binary system AM Herculis and the parameters of its components The binary system AM Herculis and the parameters of its components

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991an....312..103g&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 312, no. 2, 1991, p. 103-105.

Astronomy and Astrophysics

Astronomy

2

Binary Stars, Cataclysmic Variables, Main Sequence Stars, Stellar Mass, Stellar Spectra, White Dwarf Stars, Interstellar Gas, Stellar Magnetic Fields, Stellar Mass Accretion

Scientific paper

The parameters of the system Polar AM Herculis, the prototype star of a subgroup of cataclysmic variable binaries containing a white dwarf as primary and a low-mass main sequence star as a secondary, are reexamined. Values are given for the distance, total mass, mass function, component mass ratio, inclination angle, semimajor axis, semiminor axis of the binary system and the T(eff), M(bol), mass radius, and inclination of magnetic dipole of the components.

Affiliated with

Also associated with

No associations

Rating

The binary system AM Herculis and the parameters of its components does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The binary system AM Herculis and the parameters of its components, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The binary system AM Herculis and the parameters of its components will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1315622