248 citations · 3.6k across the 79 of their papers we have counts for
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A VLA View of the Flared, Asymmetric Disk Around the Class 0 Protostar L1527 IRS
Patrick D. Sheehan, John J. Tobin, Zhi-Yun Li +21
We present high resolution Karl G. Jansky Very Large Array (VLA) observations of the protostar L1527 IRS at 7 mm, 1.3 cm, and 2 cm wavelengths. We detect the edge-on dust disk at a…
Revisiting the Magnetic Field of the L183 Starless Core
Janik Karoly, Archana Soam, B-G Andersson +4
We present observations of linear polarization from dust thermal emission at 850 towards the starless cloud L183. These data were obtained at the James Clerk Maxwell Telescope…
Distance, magnetic field and kinematics of a filamentary cloud LDN 1157
Ekta Sharma, G. Maheswar, A. Soam +7
LDN 1157, is one of the several clouds situated in the cloud complex, LDN 1147/1158, represents a coma-shaped morphology with a well-collimated bipolar outflow emanating from a Cla…
High-resolution ALMA Study of the Proto-Brown-Dwarf Candidate L328-IRS
Chang Won Lee, Gwanjeong Kim, Philip C. Myers +6
This paper presents our observational attempts to precisely measure the central mass of a proto-brown dwarf candidate, L328-IRS, in order to investigate whether L328-IRS is in the…
How do stars gain their mass? A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star Forming Regions
Gregory J. Herczeg, Doug Johnstone, Steve Mairs +55
Most protostars have luminosities that are fainter than expected from steady accretion over the protostellar lifetime. The solution to this problem may lie in episodic mass accreti…
Extremely Energetic Outflow and Decelerated Expansion in W49N
Tie Liu, Kee-Tae Kim, Yuefang Wu +10
W49N is a mini-starburst in the Milky Way and thus an ideal laboratory for high-mass star formation studies. Due to its large distance (11.1 kpc), the kinematics in…