The Spatial Distributions of SO and N2H(+) in Taurus Molecular Cloud-1 (TMC-1)

Details The Spatial Distributions of SO and N2H(+) in Taurus Molecular Cloud-1 (TMC-1) The Spatial Distributions of SO and N2H(+) in Taurus Molecular Cloud-1 (TMC-1)

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pasj...47..845h&link_type=abstract

Publications of the Astronomical Society of Japan, v.47, p.845-851.

Astronomy and Astrophysics

Astronomy

25

Ism: Abundances, Ism: Molecules, Molecular Processes, Radio Lines: Interstellar

Scientific paper

Mapping observations were carried out toward the dark cloud, Taurus Molecular Cloud-1 (TMC-1) with the SO J_N=3_2--2_1 and N_2H(+) J=1--0 lines using the Nobeyama 45-m radiotelescope. Several local maximum positions of the SO and N_2H(+) line intensities were found in the TMC-1 ridge. The lines of SO and N_2H(+) are found to be more intense in the northwest part of the TMC-1 ridge than in the southeast part, showing that the spatial distributions of these species are rather well correlated with that of NH_3, and are anti-correlated with those of carbon-chain molecules. Based on considerations of the synthetic mechanisms of SO and N_2H(+) , their spatial distribution in TMC-1 can be explained mainly due to the differences in the chemical evolutionary stages between the northwest and southeast regions in TMC-1.

Affiliated with

Also associated with

No associations

Rating

The Spatial Distributions of SO and N2H(+) in Taurus Molecular Cloud-1 (TMC-1) 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 Spatial Distributions of SO and N2H(+) in Taurus Molecular Cloud-1 (TMC-1), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Spatial Distributions of SO and N2H(+) in Taurus Molecular Cloud-1 (TMC-1) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1563301