activity
19952023
most citedYoung Stellar Objects in the Gould Belt

303 citations · 6.9k across the 133 of their papers we have counts for

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Showing 2021Show all

9 papers · 1 filter

astro-ph.GA2021★ 23 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.CO2021★ 101 cited

CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope

Prime collaboration, M. Aravena, J. E. Austermann +84

We present a detailed overview of the science goals and predictions for the Prime-Cam direct detection camera/spectrometer being constructed by the CCAT-prime collaboration for ded…

astro-ph.EP2021★ 10 cited

Four new PLanetesimals Around TYpical and Pre-main seqUence Stars (PLATYPUS) Debris Discs at 8.8mm

Brodie J. Norfolk, Sarah T. Maddison, Jonathan P. Marshall +9

Millimetre continuum observations of debris discs can provide insights into the physical and dynamical properties of the unseen planetesimals that these discs host. The material pr…

astro-ph.EP2021★ 15 cited

A Deep Polarimetric Study of the Asymmetrical Debris Disk HD 106906

Katie A. Crotts, Brenda C. Matthews, Thomas M. Esposito +16

HD 106906 is a young, binary stellar system, located in the Lower Centaurus Crux (LCC) group. This system is unique among discovered systems in that it contains an asymmetrical deb…

astro-ph.EP2021★ 11 cited

ALMA imaging of the M-dwarf Fomalhaut C's debris disc

Patrick F. Cronin-Coltsmann, Grant M. Kennedy, Paul Kalas +9

Fomalhaut C (LP 876-10) is a low mass M4V star in the intriguing Fomalhaut triple system and, like Fomalhaut A, possesses a debris disc. It is one of very few nearby M-dwarfs known…

astro-ph.SR2021★ 4 cited

The first radio spectrum of a rapidly rotating A-type star

Jacob Aaron White, F. Tapia-Vázquez, A. G. Hughes +9

The radio spectra of main-sequence stars remain largely unconstrained due to the lack of observational data to inform stellar atmosphere models. As such, the dominant emission mech…