activity
20182022
most citedProperties of the dense core population in Orion B as seen by the Herschel Gould Belt survey

122 citations · 262 across the 5 of their papers we have counts for

collaborators

10 papers

astro-ph.GA20224 cited

Deep Herschel observations of the 2Jy sample: assessing the non-thermal and AGN contributions to the far-IR continuum

D. Dicken, C. N. Tadhunter, N. P. H. Nesvadba +5

The far-IR/sub-mm wavelength range contains a wealth of diagnostic information that is important for understanding the role of radio AGN in galaxy evolution. Here we present the re…

astro-ph.GA202123 cited

The JCMT BISTRO Survey: An 850/450m Polarization Study of NGC 2071IR in OrionB

A-Ran Lyo, Jongsoo Kim, Sarah Sadavoy +143

We present the results of simultaneous 450 m and 850 m polarization observations toward the massive star forming region NGC 2071IR, a target of the BISTRO (B-fields in Star-F…

astro-ph.GA202084 cited

Dust polarized emission observations of NGC 6334; BISTRO reveals the details of the complex but organized magnetic field structure of the high-mass star-forming hub-filament network

D. Arzoumanian, R. Furuya, T. Hasegawa +145

[Abridged] Filaments and hubs have received special attention recently thanks to studies showing their role in star formation. While the column density and velocity structures of b…

astro-ph.GA2020

Herschel Gould Belt Survey Observations of Dense Cores in the Cepheus Flare Clouds

James Di Francesco, Jared Keown, Cassandra Fallscheer +17

We present Herschel SPIRE and PACS maps of the Cepheus Flare clouds L1157, L1172, L1228, L1241, and L1251, observed by the Herschel Gould Belt Survey (HGBS) of nearby star-forming…

astro-ph.GA2020

The census of dense cores in the Serpens region from the Herschel Gould Belt Survey

E. Fiorellino, D. Elia, Ph. André +13

The Herschel Gould Belt survey mapped the nearby (d < 500 pc) star-forming regions to understand better how the prestellar phase influences the star formation process. Here we repo…

astro-ph.GA202029 cited

The accretion history of high-mass stars: An ArTéMiS pilot study of Infrared Dark Clouds

N. Peretto, A. Rigby, Ph. André +14

The mass growth of protostars is a central element to the determination of fundamental stellar population properties such as the initial mass function. Constraining the accretion h…