Massive star-formation in G24.78+0.08 studied by means of maser VLBI and thermal interferometric observations

Details Massive star-formation in G24.78+0.08 studied by means of maser VLBI and thermal interferometric observations Massive star-formation in G24.78+0.08 studied by means of maser VLBI and thermal interferometric observations

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..242..135m&link_type=abstract

Astrophysical Masers and their Environments, Proceedings of the International Astronomical Union, IAU Symposium, Volume 242, p.

Astronomy and Astrophysics

Astrophysics

Masers, Stars: Formation, Hii Regions, Techniques: Interferometric

Scientific paper

This work presents the results of VLBI observations of 6.7 GHz methanol and 22.2 GHz water masers towards the mm core A in the massive star-forming region G24.78+0.08. Comparing the maser with previous millimeter interferometric and recent continuum VLA observations, the physical properties and the gas kinematics of the G24 A core on linear scales from ~100 AU to ~0.1 pc are determined.

Affiliated with

Also associated with

No associations

Rating

Massive star-formation in G24.78+0.08 studied by means of maser VLBI and thermal interferometric observations 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 Massive star-formation in G24.78+0.08 studied by means of maser VLBI and thermal interferometric observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Massive star-formation in G24.78+0.08 studied by means of maser VLBI and thermal interferometric observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-862657