Triggered star formation on the borders of the Galactic Hii region RCW 82
نویسندگان
چکیده
منابع مشابه
The Open University ’ s repository of research publications and other research outputs Star formation triggered by the Galactic HII region RCW 120 : first results from the Herschel Space
Context. By means of different physical mechanisms, the expansion of H ii regions can promote the formation of new stars of all masses. RCW 120 is a nearby Galactic H ii region where triggered star formation occurs. This region is well-studied – there being a wealth of existing data – and is nearby. However, it is surrounded by dense regions for which far infrared data is essential to obtain an...
متن کاملThe Open University ’ s repository of research publications and other research outputs Star formation triggered by the Galactic HII region
Context. By means of different physical mechanisms, the expansion of H ii regions can promote the formation of new stars of all masses. RCW 120 is a nearby Galactic H ii region where triggered star formation occurs. This region is well-studied – there being a wealth of existing data – and is nearby. However, it is surrounded by dense regions for which far infrared data is essential to obtain an...
متن کامل’ s repository of research publications and other research outputs Star formation triggered by the Galactic HII region
Context. By means of different physical mechanisms, the expansion of H ii regions can promote the formation of new stars of all masses. RCW 120 is a nearby Galactic H ii region where triggered star formation occurs. This region is well-studied – there being a wealth of existing data – and is nearby. However, it is surrounded by dense regions for which far infrared data is essential to obtain an...
متن کاملSOAR-OSIRIS observations of the Sh 2-307 HII region: Triggered star formation beyond the solar circle
This work aims to the study of the Sh 2-307 HII region and related stellar population. Near-infrared imaging and spectroscopic observations in the direction of Sh 2-307 were performed using OSIRIS at SOAR Telescope. The photometric data were analysed from color-color, and colour-magnitude diagrams, while the spectroscopic results were interpreted from the comparison of the science spectra with ...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2008
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361:200811050