The electon temperature of AM Herculis type systems

Details The electon temperature of AM Herculis type systems The electon temperature of AM Herculis type systems

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..287w&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

Binary Stars, Cyclotron Radiation, Electron Energy, Polarized Electromagnetic Radiation, Stellar Mass Accretion, Stellar Radiation, Optical Emission Spectroscopy, Stellar Temperature, White Dwarf Stars

Scientific paper

The authors argue that the polarised optical emission from AM
Herculis-type systems arises from a compact high temperature (T ⪆ 10
keV) region closely associated with the accretion shock.

Affiliated with

Also associated with

No associations

Rating

The electon temperature of AM Herculis type systems 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 electon temperature of AM Herculis type systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The electon temperature of AM Herculis type systems will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1844122