Star formation in cooling flow galaxies

Details Star formation in cooling flow galaxies Star formation in cooling flow galaxies

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf..275c&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 275-276 (SEE N93-26706 10-90)

Astronomy and Astrophysics

Astrophysics

Cooling Flows (Astrophysics), Galaxies, Star Formation, Absorption Spectra, Elliptical Galaxies, Velocity Distribution

Scientific paper

Spectroscopic observations of central dominant galaxies are reviewed. Through the analysis of absorption spectral features (mainly the strength of the Mg triplet at 5175 A and the break in 4000 A), both in the galaxy centers and along the radii, we will be able to impose limits on the ongoing star formation as the ultimate fate for the large amounts of accreted gas. With the same aim we will carry out a dynamical study based on velocity dispersion measurements.

Affiliated with

Also associated with

No associations

Rating

Star formation in cooling flow galaxies 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 Star formation in cooling flow galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Star formation in cooling flow galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1260009