activity
19982023
most citedThe properties of brown dwarfs and low-mass hydrogen-burning stars formed by disc fragmentation

366 citations · 7.1k across the 125 of their papers we have counts for

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73 papers · 1 filter

astro-ph.GA2023★ 1 cited

ALMA-IMF IX: Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters

A. P. M. Towner, A. Ginsburg, P. Dell'Ova +24

We present a catalog of 315 protostellar outflow candidates detected in SiO J=5-4 in the ALMA-IMF Large Program, observed with ~2000 au spatial resolution, 0.339 km/s velocity reso…

astro-ph.GA2023★ 14 cited

The JCMT BISTRO Survey: Studying the Complex Magnetic Field of L43

Janik Karoly, Derek Ward-Thompson, Kate Pattle +155

We present observations of polarized dust emission at 850 m from the L43 molecular cloud which sits in the Ophiuchus cloud complex. The data were taken using SCUBA-2/POL-2 on th…

astro-ph.GA2023★ 4 cited

Line emission from filaments in molecular clouds

F. D. Priestley, D. Arzoumanian, A. P. Whitworth

Filamentary structures are often identified in column density maps of molecular clouds, and appear to be important for both low- and high-mass star formation. Theoretically, these…

astro-ph.GA2023★ 11 cited

First BISTRO observations of the dark cloud Taurus L1495A-B10: the role of the magnetic field in the earliest stages of low-mass star formation

Derek Ward-Thompson, Janik Karoly, Kate Pattle +155

We present BISTRO Survey 850 μm dust emission polarisation observations of the L1495A-B10 region of the Taurus molecular cloud, taken at the JCMT. We observe a roughly triangular n…

astro-ph.GA2023★ 10 cited

Do simulated molecular clouds look like real ones?

F. D. Priestley, P. C. Clark, A. P Whitworth

Simulations of molecular clouds often begin from highly idealised initial conditions, such as a uniform-density sphere with an artificially imposed turbulent velocity field. While…

astro-ph.GA2023★ 51 cited

ALMA-IMF. V. Prestellar and protostellar core populations in the W43 cloud complex

T. Nony, R. Galvan-Madrid, F. Motte +24

The origin of the stellar initial mass function (IMF) and its relation with the core mass function (CMF) are actively debated issues with important implications in astrophysics. Re…