Other
Scientific paper
Nov 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978phdt.........9r&link_type=abstract
Ph.D. Thesis Case Western Reserve Univ., Cleveland, OH.
Other
7
Density (Mass/Volume), Dwarf Stars, Kinematics, Luminosity, M Stars, Spectrum Analysis
Scientific paper
An objective prism survey in the red spectral region was completed which covers approximately two percent of the sky at intermediate south galactic latitudes to a limiting magnitude of V-12 for early M stars and to V-14 for late M stars. More than five hundred late K stars and M stars were detected, of which the vast majority are dwarfs. Upper and lower limits for the luminosity function for early M stars are derived from photographically determined apparent magnitudes and absolute magnitudes obtained from objective prism spectral types. The solar motion is computed from the tangential velocities of the late M dwarfs. The kinematic properties of the late M dwarfs are compared with those determined in other investigations. Some problems associated with the use of objective prism surveys in the red spectral region for the accurate classification of late main-sequence stars are presented.
No associations
LandOfFree
The kinematics and space density of M dwarf stars 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 The kinematics and space density of M dwarf stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The kinematics and space density of M dwarf stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1068101