Stellar mass spectrum in the solar neighborhood from catalogs in the astronomical data center file

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

2

Stellar Evolution, Stellar Mass, Stellar Spectra, Astronomical Catalogs, Main Sequence Stars, Star Formation Rate, Supernovae

Scientific paper

Empirical mass spectra for solar-neighborhood stars are obtained from data for 17,000 stars in eight different star catalogs. It is found that the star-formation rate has been gradually diminishing with time, while a power law with an exponent of about -2.3 fits the initial mass function for stars from 1-75 solar masses. When mass spectra are constructed from independent samples of stars, with the mass obtained by different methods, the spectrum is found to show a deficiency of stars in the 1.5-2.5 solar masses interval and possibly also in the 5-6 solar masses interval. It is concluded that these results of mass spectra indicate a type II supernova rate consistent with previous estimates.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Stellar mass spectrum in the solar neighborhood from catalogs in the astronomical data center file 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 Stellar mass spectrum in the solar neighborhood from catalogs in the astronomical data center file, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar mass spectrum in the solar neighborhood from catalogs in the astronomical data center file will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1032051

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.