The 3S0114+65 and its peculiar companion

Details The 3S0114+65 and its peculiar companion The 3S0114+65 and its peculiar companion

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..473v&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X ray Astronomy. Volume 1: X ray Binaries p 473-475 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

8

Astronomical Spectroscopy, Light Curve, X Ray Binaries, X Ray Spectroscopy, Balmer Series, Companion Stars, H Lines, Stellar Spectra, Variability

Scientific paper

A series of spectra of the optical counterpart of 3S0114+65, taken in November 1986, show a sudden increase of a factor three in the equivalent widths of the hydrogen lines. Spectra taken in 1987 show only mild variability, such as changes in the line profiles of the hydrogen lines. EXOSAT observations of the source show a variable X-ray intensity. The spectrum is hard, with variable adsorption. The possible pulse period of 14.9 minutes is not confirmed. The nature of 3S0114+65 remains unclear.

Affiliated with

Also associated with

No associations

Rating

The 3S0114+65 and its peculiar companion 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 3S0114+65 and its peculiar companion, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 3S0114+65 and its peculiar companion will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1614697