Initial jeans mass spectra of the three modes of galactic star formation: A theoretical model

Details Initial jeans mass spectra of the three modes of galactic star formation: A theoretical model Initial jeans mass spectra of the three modes of galactic star formation: A theoretical model

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26at....6..221z&link_type=abstract

Astronomical and Astrophysical Transactions (ISSN 1055-6796), vol. 6, no. 3, p. 221-228

Astronomy and Astrophysics

Astrophysics

1

Astronomical Models, Gravitational Effects, Interstellar Matter, Jeans Theory, Mass Spectra, Milky Way Galaxy, Stability, Star Formation, Galactic Evolution, Mathematical Models, Spatial Distribution

Scientific paper

We consider the problem of the gravitational instability of gas-dust matter characterized by different spatial distributions consistent with the age of the Galaxy, within the framework of the active phases theory of the Galaxy. Analytical methods are used to obtain the initial mass spectra of the Jeans fragments belonging to the spherical, intermediate and disk components of the Galaxy.

Affiliated with

Also associated with

No associations

Rating

Initial jeans mass spectra of the three modes of galactic star formation: A theoretical model 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 Initial jeans mass spectra of the three modes of galactic star formation: A theoretical model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Initial jeans mass spectra of the three modes of galactic star formation: A theoretical model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-881553