A proper-motion membership analysis of stars in the vicinity of the Orion Nebula

Details A proper-motion membership analysis of stars in the vicinity of the Orion Nebula A proper-motion membership analysis of stars in the vicinity of the Orion Nebula

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....97.1427m&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 97, May 1989, p. 1427-1439.

Other

28

Orion Nebula, Star Distribution, Stellar Motions, Astronomical Catalogs, Color-Magnitude Diagram, Emission Spectra

Scientific paper

Proper-motion membership probabilities are given for 630 stars located in the vicinity of the Orion Nebula. The region studied is roughly centered on the Trapezium and covers approximately 7 sq deg. It excludes the central 0.5 sq deg of bright nebula emission. Outsdide the emission region, accurate proper motions are available for 630 stars brighter than B = 14.0. This work, combined with other proper-motion membership analyses, provides rather comaplete membership data for the brighter stars located in the direction of the Orion Nebula.

Affiliated with

Also associated with

No associations

Rating

A proper-motion membership analysis of stars in the vicinity of the Orion Nebula 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 proper-motion membership analysis of stars in the vicinity of the Orion Nebula, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A proper-motion membership analysis of stars in the vicinity of the Orion Nebula will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1874007