The 805 second X-ray pulsar H2252-035

Details The 805 second X-ray pulsar H2252-035 The 805 second X-ray pulsar H2252-035

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...249l..25w&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 249, Oct. 1, 1981, p. L25-L28.

Astronomy and Astrophysics

Astrophysics

41

Binary Stars, Pulsars, X Ray Sources, X Ray Stars, Astronomical Models, Neutron Stars, Spectral Line Width, Stellar Models, Stellar Rotation

Scientific paper

It is shown that the X-ray flux from the 3.6 hr binary system H2252-035 is modulated at a period of 805 sec, and that its spectrum is consistent with either (1) a 1.4 photon index power law, or (2) a greater-than-20-keV thermal model. A 560 + or - 350 eV equivalent-width iron line at about 6.7 keV is noted, and the possibility that the H2252-035 system contains a slowly rotating neutron star is discussed.

Affiliated with

Also associated with

No associations

Rating

The 805 second X-ray pulsar H2252-035 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 805 second X-ray pulsar H2252-035, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 805 second X-ray pulsar H2252-035 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1468683