Chemical enrichment by tidally disrupted stars near a black hole in the Galactic Center

Details Chemical enrichment by tidally disrupted stars near a black hole in the Galactic Center Chemical enrichment by tidally disrupted stars near a black hole in the Galactic Center

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aj.....99..838l&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 99, March 1990, p. 838-842.

Astronomy and Astrophysics

Astrophysics

9

Black Holes (Astronomy), Galactic Nuclei, Interstellar Chemistry, Isotopic Enrichment, Milky Way Galaxy, Nuclear Astrophysics, Nuclear Fusion, Aluminum 26, Aluminum 27, Baryons, Dark Matter, Magnesium Isotopes, Nitrogen Isotopes, Nitrogen 15, Stellar Orbits

Scientific paper

The amount of species produced in the nucleosynthesis tidally induced by
a large black hole on infalling stars is computed. The total mass of
isotopic species N-14, N-15, Mg-25, Mg-26, and Al-26, Al-27 produced in
this process along the first billion years of the Galaxy life are
compared to possible observational evidences.

Affiliated with

Also associated with

No associations

Rating

Chemical enrichment by tidally disrupted stars near a black hole in the Galactic Center 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 Chemical enrichment by tidally disrupted stars near a black hole in the Galactic Center, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemical enrichment by tidally disrupted stars near a black hole in the Galactic Center will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1885820