The impact of mergers in the white dwarf mass distribution

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

White Dwarfs, Stellar Evolution, Spectroscopy, Galaxies, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Spectroscopy And Spectrophotometry, Galactic Center, Bar, Circumnuclear Matter, And Bulge

Scientific paper

The study of the white dwarf mass distribution gives a unique opportunity to obtain information about the amount of mass lost during stellar evolution. Spectroscopic observations of a large number of white dwarfs has allowed to derive the observational white dwarf mass distribution with accuracy. This distribution shows a central peak around the value 0.6 Msolar, but presents also a small peak at larger masses. Our purpose in this work is to evaluate the influence of the mergers of white dwarfs in the mass distribution, since it has been proved that the merging of two white dwarfs leads to a more massive white dwarf, and this mechanism might be one of the responsibles of the excess of massive white dwarfs in the white dwarf mass distribution.

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

The impact of mergers in the white dwarf mass distribution 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 impact of mergers in the white dwarf mass distribution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The impact of mergers in the white dwarf mass distribution will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1158058

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