112 citations · 973 across the 66 of their papers we have counts for
7 papers · 1 filter
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- V. Hierarchical fragmentation and gas dynamics in IRDC G034.43+00.24
Hong-Li Liu, Anandmayee Tej, Tie Liu +35
We present new 3-mm continuum and molecular lines observations from the ATOMS survey towards the massive protostellar clump, MM1, located in the filamentary infrared dark cloud (IR…
Estimating , radius and luminosity of M-dwarfs using high resolution optical and NIR spectral features
Dhrimadri Khata, Soumen Mondal, Ramkrishna Das +1
We estimate effective temperature (), stellar radius, and luminosity for a sample of 271 M-dwarf stars (M0V-M7V) observed as a part of CARMENES (Calar Alto high-Resolu…
Lynds Bright Nebulae: Sites of possible twisted filaments and ongoing star formation
L. K. Dewangan, J. S. Dhanya, N. K. Bhadari +2
The paper presents an analysis of multi-wavelength data of two Lynds Bright Nebulae (LBN), LBN 140.07+01.64 and LBN 140.771.42. The 1420 MHz continuum map reveals an extended Y-…
Clustering of low mass stars around Herbig Be star IL Cep -- Evidence of "Rocket Effect" using Gaia EDR3 ?
R. Arun, Blesson Mathew, G. Maheswar +7
We study the formation and the kinematic evolution of the early type Herbig Be star IL Cep and its environment. The young star is a member of the Cep OB3 association, at a distance…
An ALMA study of outflow parameters of protoclusters: outflow feedback to maintain the turbulence
T. Baug, Ke Wang, Tie Liu +14
With the aim of understanding the role of outflows in star formation, we performed a statistical study of the physical parameters of outflows in eleven massive protoclusters associ…
ALMA discovery of a dual dense probably rotating outflow from a massive young stellar object G18.88MME
I. I. Zinchenko, L. K. Dewangan, T. Baug +2
We report the discovery of a very dense jet-like fast molecular outflow surrounded by a wide-angle wind in a massive young stellar object (MYSO) G18.88MME (stellar mass 8 M$_…