activity
20062026
most citedThe JCMT BISTRO Survey: The magnetic field strength in the Orion A filament

144 citations · 1.3k across the 50 of their papers we have counts for

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Showing 2019Show all

12 papers · 1 filter

astro-ph.SR2019

Dust Polarization Toward Embedded Protostars in Ophiuchus with ALMA. III. Survey Overview

Sarah I. Sadavoy, Ian W. Stephens, Philip C. Myers +7

We present 0.25 arcsec resolution (35 au) ALMA 1.3 mm dust polarization observations for 37 young stellar objects (YSOs) in the Ophiuchus cloud. These data encompass all the embedd…

astro-ph.GA2019

Magnetic fields in the infrared dark cloud G34.43+0.24

Archana Soam, Tie Liu, B-G Andersson +11

We present the B-fields mapped in IRDC G34.43+0.24 using 850\,m polarized dust emission observed with the POL-2 instrument at JCMT. We examine the magnetic field geometries and…

astro-ph.GA2019

First Sub-pc Sale Mapping of Magnetic Fields in the Vicinity of a Very Low Luminosity Object, L1521F-IRS

Archana Soam, Chang Won Lee, B-G Andersson +8

L1521F is found to be forming multiple cores and it is cited as an example of the densest core with an embedded VeLLO in a highly dynamical environment. We present the core-scale m…

astro-ph.GA2019

Galactic continuum surveys with the new 850 micron MKID camera at the EAO/JCMT 15-m telescope

Tie Liu, Di Li, David Eden +24

This white paper gives a brief summary of Galactic continuum surveys with the next generation 850 micron camera at the James Clerk Maxwell Telescope (JCMT) in the next decade. This…

astro-ph.GA20193 cited

Submillimeter continuum variability in Planck Galactic cold clumps

Geumsook Park, Kee-Tae Kim, Doug Johnstone +20

In the early stages of star formation, a protostar is deeply embedded in an optically thick envelope such that it is not directly observable. Variations in the protostellar accreti…

astro-ph.GA2019

JCMT BISTRO Survey observations of the Ophiuchus Molecular Cloud: Dust grain alignment properties inferred using a Ricean noise model

Kate Pattle, Shih-Ping Lai, Tetsuo Hasegawa +18

The dependence of polarization fraction on total intensity in polarized submillimeter emission measurements is typically parameterized as , and…