Remarks on the visual binary DQ Herculis

Details Remarks on the visual binary DQ Herculis Remarks on the visual binary DQ Herculis

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91..487p&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, Aug.-Sept. 1979, p. 487-489.

Astronomy and Astrophysics

Astronomy

5

Companion Stars, Eclipsing Binary Stars, Hercules Nova, Visual Observation, Astronomical Photometry, Late Stars, Nebulae, Stellar Luminosity

Scientific paper

Photometry is reported for the eclipsing binary old nova DQ Her, its surrounding nebula, and its close visual companion. Because previous photoelectric measurements have not distinguished these components, large corrections to the published data are required. From luminosity arguments an upper limit of 0.35 solar mass for the mass of the late-type star in the eclipsing binary is derived. This appears to conflict with the spectroscopically determined mass of 0.5-0.6 solar mass.

Affiliated with

Also associated with

No associations

Rating

Remarks on the visual binary DQ Herculis 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 Remarks on the visual binary DQ Herculis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Remarks on the visual binary DQ Herculis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1487027