A5059200868- Astrophysics and Star Formation Studies
- Stellar, planetary, and galactic studies
- Regional Economic and Spatial Analysis
- Inertial Sensor and Navigation
- Molecular Spectroscopy and Structure
- Optical Systems and Laser Technology
- Astronomical Observations and Instrumentation
- Infrared Target Detection Methodologies
- Astro and Planetary Science
- Atmospheric Ozone and Climate
National Astronomical Observatories
2012
Chinese Academy of Sciences
2012
We investigate the environment of infrared dust bubble S51 and search for evidence triggered star formation in its surroundings. performed a multiwavelength study region around with data taken from large-scale surveys: 2MASS, GLIMPSE, MIPSGAL, IRAS, MALT90. analyzed spectral profile distribution molecular gas (13CO, C18O, HCN, HNC, HCO+, C2H, N2H+, HC3N), S51. used mid-infrared emission three-color image to explore physical GLIMPSE color-color diagram [5.8]-[8.0] versus [3.6]-[4.5] young...
Abstract We investigated the environment of infrared dust bubbles S51 (Zhang & Wang 2012a), N68 2012b), and N131 et al . 2012) from catalogue Churchwell (2006), searched for evidence triggered star formation.