Radial velocities of HD 187399 = V1507 Cyg

Details Radial velocities of HD 187399 = V1507 Cyg Radial velocities of HD 187399 = V1507 Cyg

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998atsir1557...19i&link_type=abstract

Astronomicheskij Tsirkulyar, no. 1557

Astronomy and Astrophysics

Astronomy

Scientific paper

HD 187399 is a spectral binary, containing a massive invisible component. Twelve spectrograms of HD 187399, obtained on the 6-meter telescope during 1982--1983, are analyzed. Radial velocities are measured for spectral lines of different elements. Balmer lines of hydrogen have a complex structure: they consist of absorption components of the B9 star and P Cyg-type profiles. As a whole, radial velocities, obtained from HeI, SiII, and MgII lines, follow the orbital curve derived by Merrill (1949).

Affiliated with

Also associated with

No associations

Rating

Radial velocities of HD 187399 = V1507 Cyg 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 Radial velocities of HD 187399 = V1507 Cyg, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radial velocities of HD 187399 = V1507 Cyg will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1721039