GINGA observations of the 6-s X-ray pulsar 1E1048.1 - 5937

Details GINGA observations of the 6-s X-ray pulsar 1E1048.1 - 5937 GINGA observations of the 6-s X-ray pulsar 1E1048.1 - 5937

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.243..553c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 243, April 15, 1990, p. 553-556.

Astronomy and Astrophysics

Astronomy

23

B Stars, Ginga Satellite, Pulsars, Satellite Observation, Stellar Mass, X Ray Binaries, Angular Momentum, Neutron Stars, X Ray Spectra

Scientific paper

From the results of Ginga observations of the X-ray pulsar 1E1048.1 -
5937, combined with previous pulse period measurements, it is found that
1E1048.1 - 5937 has exhibited secular spin-down at a rate of 4.64 + or -
1.1 x 10 to the -4th s/yr. The possibilities that this source may be
either a Be star system or a low-mass X-ray binary are considered.

Affiliated with

Also associated with

No associations

Rating

GINGA observations of the 6-s X-ray pulsar 1E1048.1 - 5937 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 GINGA observations of the 6-s X-ray pulsar 1E1048.1 - 5937, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and GINGA observations of the 6-s X-ray pulsar 1E1048.1 - 5937 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1382347