activity
20132023
most citedWhat determines the density structure of molecular clouds ? A case study of Orion B with Herschel

270 citations · 1.1k across the 22 of their papers we have counts for

collaborators

44 papers

astro-ph.GA2023

Tomographic Imaging of the Sagittarius Spiral Arm's Magnetic Field Structure

Yasuo Doi, Kengo Nakamura, Koji S. Kawabata +16

The Galactic global magnetic field is thought to play a vital role in shaping Galactic structures such as spiral arms and giant molecular clouds. However, our knowledge of magnetic…

astro-ph.GA202244 cited

On the typical width of Herschel filaments

Ph. André, P. Palmeirim, D. Arzoumanian

Herschel studies suggest that nearby (d < 500 pc) molecular filaments have a typical half-power width ~0.1pc, but this finding has been questioned on the ground that the measured w…

astro-ph.GA202212 cited

The JCMT BISTRO Survey: Multi-wavelength polarimetry of bright regions in NGC 2071 in the far-infrared/submillimetre range, with POL-2 and HAWC+

L. Fanciullo, F. Kemper, K. Pattle +31

Polarized dust emission is a key tracer in the study of interstellar medium and of star formation. The observed polarization, however, is a product of magnetic field structure, dus…

astro-ph.GA202241 cited

B-fields in Star-Forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main

Woojin Kwon, Kate Pattle, Sarah Sadavoy +149

We present 850 m polarimetric observations toward the Serpens Main molecular cloud obtained using the POL-2 polarimeter on the James Clerk Maxwell Telescope (JCMT) as part of th…

astro-ph.GA202224 cited

Velocity structure of the 50 pc-long NGC 6334 filamentary cloud: Hints of multiple compressions and their impact on the cloud properties?

Doris Arzoumanian, Delphine Russeil, Annie Zavagno +8

[Abridged] The interstellar medium is observed to be organised in filamentary structures, as well as neutral (HI) and ionized (HII) bubbles. The expanding nature of these bubbles m…

astro-ph.GA202248 cited

Filament coalescence and hub structure in MonR2: Implications to massive star and cluster formation

M. S. N. Kumar, D. Arzoumanian, A. Men'shchikov +3

Here we study the MonR2 star forming region, which has a rich network of filaments joining in a star cluster forming hub, aiming at understanding the hub structure and to examine t…