Observations of nearby M dwarf stars in VRI colors

Details Observations of nearby M dwarf stars in VRI colors Observations of nearby M dwarf stars in VRI colors

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pasp...94..821w&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 94, Oct.-Nov. 1982, p. 821-827.

Astronomy and Astrophysics

Astronomy

20

Dwarf Stars, Electrophotometry, M Stars, Stellar Color, Stellar Magnitude, Stellar Spectrophotometry, Late Stars, Star Clusters, Stellar Parallax, Variable Stars

Scientific paper

Photoelectric photometry on the Kron (1957) system is presented for 85 nearby M dwarf stars, nearly all of which have well-determined trigonometric parallaxes. For 33 stars originally observed by Kron, comparisons with the present photometry reveals some differences which may indicate significant variability for many of these stars, particularly those with hydrogen emission. The main sequence defined in the M(v), R-I plane by this sample biased toward higher proper motion lies about 0.5 m below the lower main sequence of the Hyades cluster.

Affiliated with

Also associated with

No associations

Rating

Observations of nearby M dwarf stars in VRI colors 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 Observations of nearby M dwarf stars in VRI colors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of nearby M dwarf stars in VRI colors will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1032033