A photometric and spectroscopic study of the early-type binary V1182 Aquilae

Details A photometric and spectroscopic study of the early-type binary V1182 Aquilae A photometric and spectroscopic study of the early-type binary V1182 Aquilae

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.225..961b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 225, April 15, 1987, p. 961-983.

Astronomy and Astrophysics

Astronomy

15

Binary Stars, Early Stars, Stellar Evolution, Stellar Spectrophotometry, Stellar Mass, Stellar Structure, Stellar Temperature

Scientific paper

The authors present new Strömgren photometry and medium-dispersion spectroscopy of the early-type binary V1182 Aql. The masses and radii of the two components are found to be (37.8±1.6) and (13.5±0.5) solar masses and (8.8±0.2) and (5.9±0.1) solar radii, respectively. A lower limit to the primary temperature has been established and interpretation of the evolutionary status of the system is closely linked to the adopted primary temperature.

Affiliated with

Also associated with

No associations

Rating

A photometric and spectroscopic study of the early-type binary V1182 Aquilae 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 A photometric and spectroscopic study of the early-type binary V1182 Aquilae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A photometric and spectroscopic study of the early-type binary V1182 Aquilae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1349302