activity
20002026
most citedThe Chandra Source Catalog

567 citations · 3.5k across the 87 of their papers we have counts for

collaborators
Showing 2009Show all

6 papers · 1 filter

astro-ph.GA2009★ 28 cited

The Highest Resolution Chandra View of Photoionization and Jet-Cloud Interaction in the Nuclear Region of NGC 4151

Junfeng Wang, G. Fabbiano, M. Karovska +4

We report high resolution imaging of the nucleus of the Seyfert 1 galaxy NGC 4151 obtained with a 50 ks Chandra HRC observation. The HRC image resolves the emission on spatial scal…

astro-ph.SR2009★ 95 cited

Numerical Simulations of Wind Accretion in Symbiotic Binaries

M. de Val-Borro, M. Karovska, D. Sasselov

We study the dynamical effects of gravitational focusing by a binary companion on winds from late-type stars. In particular, we investigate the mass transfer and formation of accre…

astro-ph.IM2009★ 1 cited

Active Galactic Nuclei and their role in Galaxy Formation and Evolution

Steve Kraemer, Rogier Windhorst, Kenneth G. Carpenter +3

There are several key open questions as to the nature and origin of AGN including: 1) what initiates the active phase, 2) the duration of the active phase, and 3) the effect of the…

astro-ph.SR2009★ 1 cited

Mass Transport Processes and their Roles in the Formation, Structure, and Evolution of Stars and Stellar Systems

Kenneth G. Carpenter, Margarita Karovska, Carolus J. Schrijver +15

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

astro-ph.SR2009★ 23 cited

Long-Period Variability in o Ceti

Matthew R. Templeton, Margarita Karovska

We carried out a new and sensitive search for long-period variability in the prototype of the Mira class of long-period pulsating variables, o Ceti (Mira A), the closest and bright…

astro-ph.SR2009★ 1 cited

Quantifying Stellar Mass Loss with High Angular Resolution Imaging

Stephen Ridgway, Jason Aufdenberg, Michelle Creech-Eakman +7

Mass is constantly being recycled in the universe. One of the most powerful recycling paths is via stellar mass-loss. All stars exhibit mass loss with rates ranging from ~10(-14) t…