K. K. Mallick

TL;DR: In this paper, a multi-wavelength study of the W40 star-forming region using infrared (IR) observations in the UKIRT JHK bands, Spitzer Infrared Array Camera bands, and Herschel PACS bands, 2.12 μm H{sub 2} narrowband imaging, and radio continuum observations from GMRT (610 and 1280 MHz), in a field of view (FoV) of ∼34' × 40'.

TL;DR: In this paper, the authors carried out an extensive multi-wavelength study to investigate the star formation process in the S235 complex, and they found that the Bolocam clump masses increase as we move away from the location of the ionizing star and that the molecular outflows are detected in these three subregions, further confirming the ongoing star formation activity.

TL;DR: In this paper, the authors present an analysis of multi-wavelength observations from various data sets and Galactic plane surveys to study the star-formation process in the W42 complex.

TL;DR: In this paper, a multi-wavelength study of W40 star-forming region using IR observations in UKIRT JHK bands, Spitzer IRAC bands & Herschel PACS bands; 2.12 micron H2 narrow-band imaging; and radio observations from GMRT (610 and 1280 MHz), in a FoV of ~34'x40'.

TL;DR: In this article, a combination of NIR and MIR data was used to identify 7 Class I and 133 Class II sources in the IRAS 16148−5011 region.