Helium cyclotron emission from accreting magnetized neutron stars

Details Helium cyclotron emission from accreting magnetized neutron stars Helium cyclotron emission from accreting magnetized neutron stars

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...121l...1a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 121, no. 1, May 1983, p. L1-L3.

Astronomy and Astrophysics

Astrophysics

1

Cyclotron Radiation, Helium, Magnetic Stars, Neutron Stars, Stellar Mass Accretion, Stellar Radiation, X Ray Sources, Emission Spectra, Iue, Line Spectra, Stellar Spectrophotometry, Ultraviolet Radiation

Scientific paper

The authors find that helium nuclei accreting onto magnetized neutron
stars in strong X-ray sources can emit cyclotron radiation. In the case
of the X-ray source 4U 0115+63, the He cyclotron line at 6 eV in the
ultraviolet should be observable with the IUE satellite.

Affiliated with

Also associated with

No associations

Rating

Helium cyclotron emission from accreting magnetized neutron stars 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 Helium cyclotron emission from accreting magnetized neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Helium cyclotron emission from accreting magnetized neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1585127