Other
Scientific paper
Feb 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87...89j&link_type=abstract
Astronomical Society of the Pacific, Publications, vol. 87, Feb. 1975, p. 89-95. Research supported by the Lockheed Independent
Other
11
Astronomical Catalogs, Galactic Structure, Stellar Luminosity, Supernova Remnants, B Stars, H Ii Regions, Interstellar Matter, Milky Way Galaxy, Nebulae, O Stars, Optical Properties, Root-Mean-Square Errors
Scientific paper
It is shown that luminous stars should be expected in the vicinity of supernova remnants. Luminous stars within the maximum optical areas of supernova remnants are tabulated from catalogs, and an excitation parameter is correlated with the spectral classification of such stars when their UV flux excites H II regions to produce nebular thermal bremsstrahlung. The correlations indicate that the presence of a ZAMS star of type 08 to 05 is necessary to produce thermal bremsstrahlung equal to the observed flux density at 1 GHz. Optical components of seven other supernova remnants are discussed, and it is concluded that gross uncertainties in the distance moduli of both stars and supernova remnants prevent any associations from being made.
No associations
LandOfFree
Luminous stars in galactic supernova remnants 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 Luminous stars in galactic supernova remnants, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Luminous stars in galactic supernova remnants will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1000167