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19982023
most citedSpiral Density Waves in a Young Protoplanetary Disk

346 citations · 6k across the 98 of their papers we have counts for

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Showing 2021Show all

7 papers · 1 filter

astro-ph.GA2021

The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope

P. Scicluna, F. Kemper, I. McDonald +89

The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of 850 Galactic evolved stars within 3\,kpc at (sub-)mm wavelengths, observed in the CO (21) and…

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.EP2021★ 22 cited

Low levels of sulphur dioxide contamination of Venusian phosphine spectra

Jane S. Greaves, Paul B. Rimmer, Anita M. S. Richards +7

New analysis is presented of the 1.1 mm wavelength absorption lines in Venus' atmosphere that suggested the presence of phosphine. We retrieve a sulphur dioxide observation from th…

astro-ph.GA2021★ 19 cited

Submillimetre observations of the two-component magnetic field in M82

Kate Pattle, Walter K. Gear, Matt Redman +2

We observed the starburst galaxy M82 in 850m polarised light with the POL-2 polarimeter on the James Clerk Maxwell Telescope (JCMT). We interpret our observed polarisation geome…

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.EP2021★ 37 cited

Recovery of Spectra of Phosphine in Venus' Clouds

Jane S. Greaves, Anita M. S. Richards, William Bains +7

We recover PH3 in the atmosphere of Venus in data taken with ALMA, using three different calibration methods. The whole-planet signal is recovered with 5.4σ confidence using Venus…