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20122021
most citedThe JCMT BISTRO Survey: The magnetic field strength in the Orion A filament

144 citations · 596 across the 9 of their papers we have counts for

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Showing 2018Show all

7 papers · 1 filter

astro-ph.GA2018

JCMT BISTRO survey: Magnetic Fields within the Hub-Filament Structure in IC 5146

Jia-Wei Wang, Shih-Ping Lai, Chakali Eswaraiah +130

We present the 850 m polarization observations toward the IC5146 filamentary cloud taken using the Submillimetre Common-User Bolometer Array 2 (SCUBA-2) and its associated polar…

astro-ph.SR2018

ALMA detections of the youngest protostars in Ophiuchus

Rachel K. Friesen, Andy Pon, Tyler L. Bourke +4

We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of 1.1 mm dust continuum and CO 2-1 emission toward six dense cores within the Ophiuchus molecular cloud…

astro-ph.GA2018

Kinematics of dense gas in the L1495 filament

A. Punanova, P. Caselli, J. E. Pineda +4

We study the kinematics of the dense gas of starless and protostellar cores traced by the N2D+(2-1), N2H+(1-0), DCO+(2-1), and H13CO+(1-0) transitions along the L1495 filament and…

astro-ph.GA2018

Magnetic fields towards Ophiuchus-B derived from SCUBA-2 polarization measurements

Archana Soam, Kate Pattle, Derek Ward-Thompson +121

We present the results of dust emission polarization measurements of Ophiuchus-B (Oph-B) carried out using the Submillimetre Common-User Bolometer Array 2 (SCUBA-2) camera with its…

astro-ph.GA2018

A First Look at BISTRO Observations of The Oph-A core

Jungmi Kwon, Yasuo Doi, Motohide Tamura +119

We present 850 m imaging polarimetry data of the Oph-A core taken with the Submillimeter Common-User Bolometer Array-2 (SCUBA-2) and its polarimeter (POL-2), as part of our…

astro-ph.GA2018

Seeds of Life in Space (SOLIS). III. Zooming into the methanol peak of the pre-stellar core L1544

Anna Punanova, Paola Caselli, Siyi Feng +41

Towards the pre-stellar core L1544, the methanol (CHOH) emission forms an asymmetric ring around the core centre, where CHOH is mostly in solid form, with a clear peak 4000…