G29.96-0.02 and G35.20-1.74 1mm and 3mm maps (Pillai+, 2011)

Details G29.96-0.02 and G35.20-1.74 1mm and 3mm maps (Pillai+, 2011) G29.96-0.02 and G35.20-1.74 1mm and 3mm maps (Pillai+, 2011)

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35309118p&link_type=abstract

VizieR On-line Data Catalog: J/A+A/530/A118. Originally published in: 2011A&A...530A.118P

Physics

Molecular Clouds, Millimetric/Submm Sources, Radio Continuum

Scientific paper

Most work on high-mass star formation has focused on observations of young massive stars in protoclusters. Very little is known about the preceding stage. Here, we present a new high-resolution study of pre-protocluster regions in tracers exclusively probing the coldest and dense gas (NH2 D). The two target regions G29.96-0.02 and G35.20-1.74 (W48) are drawn from the SCAMPS project, which searches for pre-protoclusters near known ultracompact HII regions. We used our data to constrain the chemical, thermal, kinematic, and physical conditions (i.e., densities) in G29.96e and G35.20w. NH3, NH2 D, HCO+, and continuum emission were mapped using the VLA, PdBI, and BIMA.
(2 data files).

Affiliated with

Also associated with

No associations

Rating

G29.96-0.02 and G35.20-1.74 1mm and 3mm maps (Pillai+, 2011) 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 G29.96-0.02 and G35.20-1.74 1mm and 3mm maps (Pillai+, 2011), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and G29.96-0.02 and G35.20-1.74 1mm and 3mm maps (Pillai+, 2011) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1208419