The shell spectrum of the optical counterpart of GX 304-1 /4U 1258-61/

Details The shell spectrum of the optical counterpart of GX 304-1 /4U 1258-61/ The shell spectrum of the optical counterpart of GX 304-1 /4U 1258-61/

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.190..537p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 190, Feb. 1980, p. 537-542. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

28

B Stars, Companion Stars, Dwarf Stars, Stellar Evolution, Stellar Spectra, Distance, H Lines, Stellar Envelopes, Stellar Mass Ejection, X Ray Stars

Scientific paper

A high-resolution spectrum of the shell star associated with GX 304-1
(4U 1258 -61) has been obtained. The star is of spectral type B2 Vne. It
is rotating at near break-up velocity and losing mass, probably via an
expanding equatorial disc ˜2-5 R* in size. A distance
of 2.4 ± 0.5 kpc is derived.

Affiliated with

Also associated with

No associations

Rating

The shell spectrum of the optical counterpart of GX 304-1 /4U 1258-61/ 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 shell spectrum of the optical counterpart of GX 304-1 /4U 1258-61/, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The shell spectrum of the optical counterpart of GX 304-1 /4U 1258-61/ will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1621533