activity
20142020
most citedATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- I. Survey description and a first look at G9.62+0.19

112 citations · 184 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2020112 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- I. Survey description and a first look at G9.62+0.19

Tie Liu, Neal J. Evans, Kee-Tae Kim +41

The "ATOMS," standing for {\it ALMA Three-millimeter Observations of Massive Star-forming regions}, survey has observed 146 active star forming regions with ALMA Band 3, aiming to…

astro-ph.GA201933 cited

ALMA observations reveal no preferred outflow--filament and outflow--magnetic field orientations

T. Baug, Ke Wang, Tie Liu +12

We present a statistical study on the orientation of outflows with respect to large-scale filaments and the magnetic fields. Although filaments are widely observed toward Galactic…

astro-ph.GA20198 cited

Evidence of interacting elongated filaments in the star-forming site AFGL 5142

Lokesh K. Dewangan, Devendra K. Ojha, Tapas Baug +1

To probe the ongoing physical mechanism, we studied a wide-scale environment around AFGL 5142 (area ~25 pc x 20 pc) using a multi-wavelength approach. The Herschel column density (…

astro-ph.GA201630 cited

Star formation around mid-infrared bubble N37: Evidence of cloud-cloud collision

T. Baug, L. K. Dewangan, D. K. Ojha +1

We have performed a multi-wavelength analysis of a mid-infrared (MIR) bubble N37 and its surrounding environment. The selected 1515 area around the bubble contains two…

astro-ph.SR20141 cited

Possible spatial asymmetry in semi-regular variable UZ Arietis

Tapas Baug, T. Chandrasekhar, Shashikiran Ganesh

Semi-regular variables (SRVs) though closely related to Mira variables, are a less studied class of AGB stars. While asymmetry in the brightness distribution of many Mira variables…