Chemical model for dense portion of the nearby globule Barnard (B68)

Details Chemical model for dense portion of the nearby globule Barnard (B68) Chemical model for dense portion of the nearby globule Barnard (B68)

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005newa...11..138a&link_type=abstract

New Astronomy, Volume 11, Issue 2, p. 138-145.

Astronomy and Astrophysics

Astronomy

98.58.Db

Scientific paper

We have studied the chemistry of the isolated globule Barnard (B68). The chemical evolution is studied using pseudo-time-dependent and contracting models, involving pure gas-phase and gas-grain chemistry. Our results confirm the importance of grain chemistry in predicting the observed species in B68. We have also outlined the impact of using contracting models on producing more reliable results of the chemical evolution of the dark clouds such as B68.

Affiliated with

Also associated with

No associations

Rating

Chemical model for dense portion of the nearby globule Barnard (B68) 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 model for dense portion of the nearby globule Barnard (B68), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemical model for dense portion of the nearby globule Barnard (B68) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1651866