Spectral variability of the massive X-ray binary LSI +65(deg) 010

Details Spectral variability of the massive X-ray binary LSI +65(deg) 010 Spectral variability of the massive X-ray binary LSI +65(deg) 010

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...350..855l&link_type=abstract

Astronomy and Astrophysics, v.350, p.855-858 (1999)

Astronomy and Astrophysics

Astrophysics

4

Line: Profiles, Stars: Individual: Lsi +65(Deg) 010, Stars: Supergiants, X-Rays: Stars

Scientific paper

We present optical spectroscopic observations of the massive X-ray binary LSI +65(deg) 010, the optical counterpart to the X-ray transient 2S0114+65. Our data show a dramatic variability in 1992 and only a mild variability during 1993-1995. An increase by a factor more than three in the equivalent width of the Hα emission line within four days is present in Nov. 1992. It is interesting to notice that changes have taken place only in the blue side on Nov. 4, 1992, when compared to similar spectrum taken one day before. We associate this phenomenon with the existence of an HII region around the neutron star. A double-peak profile is seen in the spectrum of Sept. 1994. If this double-peak profile is real, we suggest that such a profile may be explained by the emission line from an HII region around the neutron star, superposed on that from the stellar wind of the supergiant.

Affiliated with

Also associated with

No associations

Rating

Spectral variability of the massive X-ray binary LSI +65(deg) 010 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 Spectral variability of the massive X-ray binary LSI +65(deg) 010, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral variability of the massive X-ray binary LSI +65(deg) 010 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1081331