activity
20022020
most citedThe close circumstellar environment of Betelgeuse - V. Rotation velocity and molecular envelope properties from ALMA

82 citations · 870 across the 36 of their papers we have counts for

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Showing astro-ph.SRShow all

27 papers · 1 filter

astro-ph.SR2020★ 63 cited

The Photospheric Temperatures of Betelgeuse during the Great Dimming of 2019/2020: No New Dust Required

Graham M Harper, Edward F Guinan, Richard Wasatonic +1

The processes that shape the extended atmospheres of red supergiants (RSGs), heat their chromospheres, create molecular reservoirs, drive mass loss, and create dust remain poorly u…

astro-ph.SR2020★ 20 cited

ALMA and VLA reveal the lukewarm chromospheres of the nearby red supergiants Antares and Betelgeuse

E. O'Gorman, G. M. Harper, K. Ohnaka +8

We first present spatially resolved ALMA and VLA continuum observations of the early-M red supergiant Antares to search for the presence of a chromosphere at radio wavelengths. We…

astro-ph.SR2020★ 16 cited

SOFIA-EXES Observations of Betelgeuse during the Great Dimming of 2019/2020

Graham M. Harper, Curtis N. DeWitt, Matthew J. Richter +6

In 2019 October Betelgeuse began a decline in V-band brightness that went beyond the minimum expected from its quasi-periodic ~420 day cycle, becoming the faintest in recorded phot…

astro-ph.SR2019

Stars at High Spatial Resolution

Kenneth G. Carpenter, Gerard van Belle, Alexander Brown +19

We summarize some of the compelling new scientific opportunities for understanding stars and stellar systems that can be enabled by sub-milliarcsec (sub-mas) angular resolution, UV…

astro-ph.SR2019★ 28 cited

NOEMA maps the CO environment of the red supergiant Cep

M. Montargès, W. Homan, D. Keller +8

Red supergiant stars are surrounded by a gaseous and dusty circumstellar environment created by their mass loss which spreads heavy elements into the interstellar medium. The struc…

astro-ph.SR2019

Astro2020: Molecular Masers as Probes of the Dynamic Atmospheres of Dying Stars

Lynn D. Matthews, Mark J Claussen, Graham M. Harper

More than half of the dust and heavy element enrichment in galaxies originates from the winds and outflows of evolved, low-to-intermediate mass stars on the asymptotic giant branch…