Molecular Gas Distribution and Kinematics of the Starless Core L1521F

Details Molecular Gas Distribution and Kinematics of the Starless Core L1521F Molecular Gas Distribution and Kinematics of the Starless Core L1521F

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999sf99.proc..179l&link_type=abstract

Star Formation 1999, Proceedings of Star Formation 1999, held in Nagoya, Japan, June 21 - 25, 1999, Editor: T. Nakamoto, Nobeyam

Physics

Scientific paper

We present CS, CCS and N2H+ observations of the starless core, L1521F in the Taurus Molecular Cloud (TMC). The CCS emission traces the outer 0.1pc envelope of the core while the N2H+ emission traces the inner 0.05pc region. CCS kinematics suggests both infall and rotation motions while the N2H+ kinematics suggests only rotation motion. CCS and N2H+ rotation are apparently in the opposite direction, suggesting that the inner and outer regions are kinematically decoupled and that the inner region may have yet to experience infall.

Affiliated with

Also associated with

No associations

Rating

Molecular Gas Distribution and Kinematics of the Starless Core L1521F 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 Molecular Gas Distribution and Kinematics of the Starless Core L1521F, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Molecular Gas Distribution and Kinematics of the Starless Core L1521F will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1061369