Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...259..677t&link_type=abstract
Astrophysical Journal, Part 1, vol. 259, Aug. 15, 1982, p. 677-692.
Astronomy and Astrophysics
Astronomy
39
F Stars, Stellar Coronas, Stellar Luminosity, X Ray Astronomy, Dwarf Stars, Giant Stars, Maximum Likelihood Estimates, Tables (Data)
Scientific paper
An X-ray survey has been conducted of stars brighter than visual magnitude 8.5 that have serendipitously fallen into the fields of view of the Imaging Proportional Counter of the Einstein Observatory. The survey includes 227 separate 1 x 1 deg fields, containing 274 stars with a visual magnitude of no more than 8.5 and covering a wide range of spectral types and luminosity classes. X-ray emission was detected from 33 stars, and upper limits have been determined for the remainder of the sample. F type stars dominate the detected sample, and most of these are shown to be dwarfs. An X-ray luminosity function for dF stars has been deduced, and reveals that the average 0.2-4.0 keV luminosity of these stars is around 10 to the 29th erg/sec. Constraints have been placed on the high luminosity tails and medians of the X-ray luminosity functions for other types of stars.
Avni Yoav
Golub Leon
Gorenstein Paul
Harnden Frank R. Jr.
Rosner Robert
No associations
LandOfFree
A magnitude limited stellar X-ray survey and the F star X-ray luminosity function 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 magnitude limited stellar X-ray survey and the F star X-ray luminosity function, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A magnitude limited stellar X-ray survey and the F star X-ray luminosity function will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-899852