112 citations · 1.8k across the 72 of their papers we have counts for
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Unveiling the importance of magnetic fields in the evolution of dense clumps formed at the waist of bipolar H II regions: a case study on Sh2-201 with JCMT SCUBA-2/POL-2
Chakali Eswaraiah, Di Li, Manash R. Samal +10
We present the properties of magnetic fields (B-fields) in two clumps (clump 1 and clump 2), located at the waist of the bipolar H II region Sh2-201, based on JCMT SCUBA-2/POL-2 ob…
Multiwavelength Polarimetry of the Filamentary Cloud IC5146: II. Magnetic Field Structures
Jia-Wei Wang, Shih-Ping Lai, Dan P. Clemens +4
The IC5146 cloud is a nearby star-forming region in Cygnus, consisting of molecular gas filaments in a variety of evolutionary stages. We used optical and near-infrared polarizatio…
Polarimetric and photometric investigation of a dark globule LDN 1225: distance, extinction law, and magnetic fields
Chakali Eswaraiah, Shih-Ping Lai, Yuehui Ma +7
We present the results based on the optical -band polarization observations of 280 stars distributed towards the dark globule LDN\,1225. {\it Gaia} data release 2 parallaxes alo…
Star formation in the Sh 2-53 region influenced by accreting molecular filaments
T. Baug, L. K. Dewangan, D. K. Ojha +6
We present a multi-wavelength analysis of a 3030 area around the Sh 2-53 region (hereafter S53 complex), which is associated with at least three H II regions, tw…
Multi-wavelength Stellar Polarimetry of the Filamentary Cloud IC5146: I. Dust Properties
Jia-Wei Wang, Shih-Ping Lai, C. Eswaraiah +3
We present optical and near-infrared stellar polarization observations toward the dark filamentary clouds associated with IC5146. The data allow us to investigate the dust properti…
Understanding the links among magnetic fields, filament, the bipolar bubble, and star formation in RCW57A using NIR polarimetry
C. Eswaraiah, Shih-Ping Lai, Wen-Ping Chen +10
The influence of magnetic fields (B-fields) in the formation and evolution of bipolar bubbles, due to the expanding ionization fronts (I-fronts) driven by the Hii regions that are…