activity
20022023
most citedNear-UV Absorption, Chromospheric Activity, and Star-Planet Interactions in the WASP-12 system

228 citations · 1.5k across the 43 of their papers we have counts for

collaborators
Showing 2018Show all

7 papers · 1 filter

astro-ph.SR2018★ 8 cited

Constraining the magnetic field on white dwarf surfaces; Zeeman effects and fine structure constant variation

J. Hu, J. K. Webb, T. R. Ayres +12

White dwarf atmospheres are subjected to gravitational potentials around times larger than occur on Earth. They provide a unique environment in which to search for any possi…

astro-ph.SR2018★ 15 cited

The Advanced Spectral Library (ASTRAL): Reference Spectra for Evolved M-Stars

Kenneth G. Carpenter, Krister E. Nielsen, Gladys V. Kober +3

The HST Treasury Program "Advanced Spectral Library Project: Cool Stars" was designed to collect representative, high quality ultraviolet spectra of eight evolved F-M type cool sta…

astro-ph.SR2018★ 10 cited

The extreme O-type spectroscopic binary HD 93129A

D. Gruner, R. Hainich, A. A. C. Sander +6

HD 93129A was classified as the earliest O-type star in the Galaxy (O2~If*) and is considered as the prototype of its spectral class. However, interferometry shows that this object…

astro-ph.SR2018★ 3 cited

Serendipitous X-ray Sources in the Chandra HRC Field around Alpha Centauri

Thomas R. Ayres

For more than a decade, Alpha Centauri AB (G2V+K1V) has been observed by Chandra, in a long-term program to follow coronal (T~1MK) activity cycles of the two sunlike stars. Over 20…

astro-ph.SR2018★ 28 cited

First high-resolution look at the quiet Sun with ALMA at 3 mm

A. Nindos, C. E. Alissandrakis, T. S. Bastian +9

We present an overview of high resolution quiet Sun observations, from disk center to the limb, obtained with the Atacama Large mm and sub-mm Array (ALMA) at 3 mm. Seven quiet Sun…

astro-ph.SR2018★ 10 cited

Beyond the Coronal Graveyard

Thomas R. Ayres

New Chandra High Resolution Camera pointings on the "non-coronal" red giant Arcturus (HD124897; Boo: K1.5III) corroborate a tentative soft X-ray detection in a shorter explorat…