The Stellar Birthline and Birth-Rate Function in IC 1805: A Feasibility Study

Details The Stellar Birthline and Birth-Rate Function in IC 1805: A Feasibility Study The Stellar Birthline and Birth-Rate Function in IC 1805: A Feasibility Study

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.1503k&link_type=abstract

American Astronomical Society Meeting 205, #15.03; Bulletin of the American Astronomical Society, Vol. 36, p.1362

Astronomy and Astrophysics

Astronomy

Scientific paper

HR diagrams for the youngest, optically-visible clusters potentially encode (a) the range of mass accretion rates, dM/dt, that characterized the stellar assembly phase; and (b) the rate of star formation as a function of mass, N(M,t). In this contribution, we make use of published photometry and spectroscopy for the young cluster IC 1805 to explore the factors that influence our ability to deduce dM/dt and N(M,t), and to suggest observations that could in principle provide more robust constraints on these quantities.

Affiliated with

Also associated with

No associations

Rating

The Stellar Birthline and Birth-Rate Function in IC 1805: A Feasibility Study 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 Stellar Birthline and Birth-Rate Function in IC 1805: A Feasibility Study, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Stellar Birthline and Birth-Rate Function in IC 1805: A Feasibility Study will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1635998