S
Swagat Ranjan Das
Researcher at Indian Institute of Space Science and Technology
Publications - 8
Citations - 41
Swagat Ranjan Das is an academic researcher from Indian Institute of Space Science and Technology. The author has contributed to research in topics: Star formation & Young stellar object. The author has an hindex of 4, co-authored 6 publications receiving 36 citations.
Papers
More filters
Journal ArticleDOI
Infrared dust bubble CS51 and its interaction with the surrounding interstellar medium
Swagat Ranjan Das,Anandmayee Tej,Sarita Vig,Hong-Li Liu,Hong-Li Liu,Hong-Li Liu,Tie Liu,C. H. Ishwara Chandra,Swarna K. Ghosh +8 more
TL;DR: In this paper, a multi-wavelength investigation of the southern infrared dust bubble CS51 is presented, where the associated ionized, cold dust, molecular and stellar components are investigated.
Journal ArticleDOI
Radio and infrared study of the star-forming region IRAS 20286+4105
Varsha Ramachandran,Swagat Ranjan Das,Anandmayee Tej,Sarita Vig,S. K. Ghosh,S. K. Ghosh,Devendra K. Ojha +6 more
TL;DR: In this paper, a multi-wavelength investigation of the star-forming complex IRAS 20286+4105, located in the Cygnus X region, is presented.
Journal ArticleDOI
High-mass star formation toward southern infrared bubble S10
TL;DR: In this paper, an investigation in radio and infrared wavelengths of two high-mass star forming regions toward the southern Galactic bubble S10 is presented, where the two regions under study are associated with the broken bubble S 10 and Extended Green Object, G345.
Journal ArticleDOI
High-mass star formation toward southern infrared bubble s10
Posted Content
Radio and infrared study of the star forming region IRAS 20286+4105
Varsha R,Swagat Ranjan Das,Anandmayee Tej,Sarita Vig,S. K. Ghosh,S. K. Ghosh,Devendra K. Ojha +6 more
TL;DR: In this paper, a multi-wavelength investigation of the star forming complex IRAS 20286+4105, located in the Cygnus-X region, is presented, where radio continuum observations, at 610 and 1280 MHz, show the presence of a HII region possibly powered by a star of spectral type B0 - B0.5.