activity
20042023
most citedThe UV Scattering Halo of the Central Source Associated with Eta Carinae

95 citations · 511 across the 14 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2023

Eta Carinae: the dissipating occulter is an extended structure

Theodore R. Gull, Henrik Hartman, Mairan Teodoro +10

Previous STIS long-slit observations of Eta Carinae identified numerous absorption features in both the stellar spectrum, and in the adjacent nebular spectra, along our line-of-sig…

astro-ph.SR2022

Eta Carinae: an evolving view of the central binary, its interacting winds and its foreground ejecta

Theodore R. Gull, D. John Hillier, Henrik Hartman +13

FUV spectra of Eta Car, recorded across two decades with HST/STIS, document multiple changes in resonant lines caused by dissipating extinction in our line of sight. The FUV flux h…

astro-ph.GA2020★ 13 cited

Eta Carinae & the Homunculus: Far Infrared, Sub-millimeter Spectral Lines

T. R. Gull, P. W. Morris, J. H. Black +4

The evolved massive binary star Eta Carinae underwent eruptive mass loss events that formed the complex bi-polar Homunculus nebula harboring tens of solar masses of unusually nitro…

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…