Spectroscopic and photometric observations in Bochum 10 and 11

Details Spectroscopic and photometric observations in Bochum 10 and 11 Spectroscopic and photometric observations in Bochum 10 and 11

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.228..545f&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 228, Oct. 1, 1987, p. 545-555. NSERC-supported research

Astronomy and Astrophysics

Astronomy

14

Astronomical Photometry, Astronomical Spectroscopy, Star Clusters, Stellar Spectrophotometry, Color-Magnitude Diagram, Main Sequence Stars, Stellar Color, Stellar Spectra

Scientific paper

Stars were selected for photometry in and around Bochum 10 from candidates in the general cluster region and near the BSC star HR4177, and stars in Bochum 11 were selected in the general cluster region. Bochum 10 is found to be a loose B0 cluster of about 21 stars whose members are probably brighter than M(v) = -1. The modulus and marginally variable photometric extinction are not significantly different than those found spectroscopically. Bochum 11 is shown to be a sparse cluster with a possible premain sequence and an age of roughly 0.3-3 million years. Nebulosity and variable extinction are noted in the stellar spectrum.

Affiliated with

Also associated with

No associations

Rating

Spectroscopic and photometric observations in Bochum 10 and 11 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 Spectroscopic and photometric observations in Bochum 10 and 11, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic and photometric observations in Bochum 10 and 11 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1776064