Physics
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atnf.prop.3621s&link_type=abstract
ATNF proposal V436, Semester: October, 2010
Physics
Masers (Galactic And Extragalactic), Star Formation, Lba
Scientific paper
Internal proper-motion measurements of 6.7 GHz methanol masers can provide unique information about high-mass star-forming regions (HMSFRs). The source G320.23-0.28 is the best case where the methanol masers are parallel to a large-scale bi-lobed outflow traced by H_2, SiO, and EGO emissions in the east-west direction. Therefore, it appears that the G320.23-0.28 methanol maser spatially and physically trace the outflow ejected from a high-mass YSO in early evolutionary stage. We have accurately measured the spatial distribution of the G320.23-0.28 methanol maser using the LBA (Project: v292a), and that distribution exhibited a complex spatial distribution. By applying the bipolar outflow model of Moscadelli et al. (2000, 2005) to our observed distribution, we obtained maser-outflow axis and opening angles that were consistent with the large-scale outflow. We propose to carry out three-epoch observations of the 6.7 GHz methanol masers in G320.23-0.28 to measure their internal proper motions. This measurement will provide vital information about both the location of this maser with SFRs and studies of outflows at early evolutionary stages in HMSF.
Bartkiewicz Anna
Ellingsen Simon
Fujisawa Kenta
Sugiyama Koichiro
No associations
LandOfFree
Measurement of the bipolar outflow motions of the 6.7 GHz Methanol Masers in G320.23-0.28 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 Measurement of the bipolar outflow motions of the 6.7 GHz Methanol Masers in G320.23-0.28, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Measurement of the bipolar outflow motions of the 6.7 GHz Methanol Masers in G320.23-0.28 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1120228