Searching for initial stage of massive star formation around the H II region G18.2–0.3
Creators
- 1. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 (China)
Description
Sometimes, early star formation can be found in cold and dense molecular clouds, such as an infrared dark cloud. Considering that star formation often occurs in clusters, H II regions may be triggering a new generation of star formation, so we can search for the initial stage of massive star formation around H II regions. Based on the above, this work introduces one method to search for the initial stage of massive star formation around H II regions. Towards one section of the H II region G18.2–0.3, multiwavelength observations are carried out to investigate its physical properties. Through analysis, we find three potential initial stages of massive star formation, suggesting that it is feasible to use in searching for the initial stage of massive star formation around H II regions. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1674-4527/17/6/57Additional details
Identifiers
Publishing Information
- Journal Title
- Research in Astronomy and Astrophysics
- Journal Volume
- 17
- Journal Issue
- 6
- Journal Page Range
- [12 p.]
- ISSN
- 1674-4527
INIS
- Country of Publication
- China
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 49084327
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- GALAXIES; HYDROGEN; INTERSTELLAR SPACE; MOLECULES; PHYSICAL PROPERTIES; STARS
- Descriptors DEC
- ELEMENTS; NONMETALS; SPACE