55 citations · 196 across the 14 of their papers we have counts for
14 papers
Gas kinematics and dynamics of Carina Pillars: A case study of G287.76-0.87
Ngo-Duy Tung, Le Ngoc Tram, Archana Soam +4
We study the kinematics of a pillar, namely G287.76-0.87, using three rotational lines of CO(5-4), CO(8-7), CO(11-10), and a fine structure line of [OI] $63\,μ…
investigation of cores and filamentary structures in L1251 located in the Cepheus flare
Divyansh Dewan, Archana Soam, Guo-Yin Zhang +3
Context: Molecular clouds are the prime locations of star formation. These clouds contain filamentary structures and cores which are crucial in the formation of young stars. Aims:…
Turbulence and Magnetic Fields in Star Formation
Archana Soam, Chakali Eswaraiah, Amit Seta +2
Molecular clouds are prime locations to study the process of star formation. These clouds contain filamentary structures and cores, which are crucial sites for the formation of you…
On the Scarcity of Dense Cores ( cm) in High Latitude Planck Galactic Cold Clumps
Fengwei Xu, Ke Wang, Tie Liu +34
High-latitude () molecular clouds have virial parameters that exceed 1, but whether these clouds can form stars has not been studied systematically. Using JCMT SCUB…
TRAO Survey of Nearby Filamentary Molecular clouds, the Universal Nursery of Stars (TRAO-FUNS). III. Filaments and dense cores in the NGC 2068 and NGC 2071 regions of Orion B
Hyunju Yoo, Chang Won Lee, Eun Jung Chung +9
We present the results of molecular line observations performed toward the NGC 2068 and NGC 2071 regions of the Orion B cloud as the TRAO-FUNS project to study the roles of the fil…
High Resolution Observations of HI in the IC 63 Reflection Nebula
L. Bonne, B-G Andersson, R. Minchin +7
Photodissociation regions (PDRs), where the (far-)ultraviolet light from hot young stars interact with the gas in surrounding molecular clouds, provide laboratories for understandi…