High-mass protostellar candidates (Williams+, 2004)

Details High-mass protostellar candidates (Williams+, 2004) High-mass protostellar candidates (Williams+, 2004)

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..34170115w&link_type=abstract

VizieR On-line Data Catalog: J/A+A/417/115. Originally published in: 2004A&A...417..115W

Other

1

Ysos, Interstellar Medium, Infrared Sources

Scientific paper

The sample of High-Mass Protostellar Objects (HMPOs was observed at 850{mu}m and 450{mu}m between March 2000 and June 2000 using the Submillimetre Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope. The position and measured flux of the detections resolved by our JCMT observations. Positions are measured from the 450{mu}m "jiggle" maps wherever possible. Unless otherwise stated, 450{mu}m detections without corresponding 850{mu}m detections arise from the increased resolution of the 450{mu}m observations.
(1 data file).

Affiliated with

Also associated with

No associations

Rating

High-mass protostellar candidates (Williams+, 2004) 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 High-mass protostellar candidates (Williams+, 2004), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-mass protostellar candidates (Williams+, 2004) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1030657