The optical counterpart of the X-ray burster Serpens X-1 /4U 1837+04/

Details The optical counterpart of the X-ray burster Serpens X-1 /4U 1837+04/ The optical counterpart of the X-ray burster Serpens X-1 /4U 1837+04/

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238..964t&link_type=abstract

Astrophysical Journal, Part 1, vol. 238, June 15, 1980, p. 964-968.

Astronomy and Astrophysics

Astrophysics

15

Stellar Spectrophotometry, X Ray Sources, Astronomical Photography, Electrophotometry, Stellar Luminosity, Stellar Spectra

Scientific paper

The Davidsen candidate for Serpens X-1 was resolved into two stars separated by 2.1 arcsec. One is ultraviolet and shows apparent emission at He II 4686 A; this star is identified with the X-ray source. Color limits imply an obscuration A(B) of not less than 6.2. This confirms that the X-ray to optical luminosity ratio is very large (greater than 100).

Affiliated with

Also associated with

No associations

Rating

The optical counterpart of the X-ray burster Serpens X-1 /4U 1837+04/ 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 optical counterpart of the X-ray burster Serpens X-1 /4U 1837+04/, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The optical counterpart of the X-ray burster Serpens X-1 /4U 1837+04/ will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1214762