activity
20002019
most citedHigh Mass Triple Systems: The Classical Cepheid Y Car

35 citations · 129 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2019★ 1 cited

The Potential of Exozodiacal Disks Observations with the WFIRST Coronagraph Instrument

B. Mennesson, V. Bailey, J. Kasdin +60

The Wide Field Infrared Survey Telescope (WFIRST) Coronagraph Instrument (CGI) will be the first high-performance stellar coronagraph using active wavefront control for deep starli…

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★ 9 cited

Constraining stellar parameters and atmospheric dynamics of the carbon AGB star V Oph

Gioia Rau, Keiichi Ohnaka, Markus Wittkowski +2

Molecules and dust produced by the atmospheres of cool evolved stars contribute to a significant amount of the total material found in the interstellar medium. To understand the me…

astro-ph.SR2019

Cool, evolved stars: results, challenges, and promises for the next decade

Gioia Rau, Rodolfo Montez, Kenneth G. Carpenter +27

Cool, evolved stars are the main source of chemical enrichment of the interstellar medium (ISM), and understanding their mass loss and structure offers a unique opportunity to stud…

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★ 17 cited

GHRS Observations of Cool, Low-Gravity Stars. VI Mass-Loss Rates and Wind Parameters for M Giants

Gioia Rau, Krister E. Nielsen, Kenneth G. Carpenter +1

The photon-scattering winds of M-giants absorb parts of the chromospheric emission lines and produce self-reversed spectral features in high resolution {\it HST}/GHRS spectra. Thes…