A comment on `Chemical evolution in circumstellar structure of B5 IRS1' by Kelly, Macdonald & Millar

Details A comment on `Chemical evolution in circumstellar structure of B5 IRS1' by Kelly, Macdonald & Millar A comment on `Chemical evolution in circumstellar structure of B5 IRS1' by Kelly, Macdonald & Millar

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.282..900w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 282, Issue 3, pp. 900-902.

Astronomy and Astrophysics

Astronomy

3

Stars: Formation, Ism: Abundances, Ism: General, Ism: Kinematics And Dynamics

Scientific paper

We show that the observations of Kelly, Macdonald & Millar provide a strong indication of the freeze-out of molecules on to dust, but they do not constrain the cyclic models of regions of low-mass star formation because the observed sources are the remnants of core collapse and are not in one of the phases of evolution treated in the cyclic models. We discuss observations that are needed to provide tests of the cyclic models.

Affiliated with

Also associated with

No associations

Rating

A comment on `Chemical evolution in circumstellar structure of B5 IRS1' by Kelly, Macdonald & Millar 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 A comment on `Chemical evolution in circumstellar structure of B5 IRS1' by Kelly, Macdonald & Millar, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A comment on `Chemical evolution in circumstellar structure of B5 IRS1' by Kelly, Macdonald & Millar will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1137604