activity
20232025
most citedIntroducing the Condor Array Telescope. II. Deep imaging observations of the edge-on spiral galaxy NGC 5907 and the NGC 5866 Group: yet another view of the iconic stellar stream

1 citations · 1 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025

A 70 pc-Diameter Nova Super-remnant Surrounding the Recurrent Nova RS Ophiuchi

Michael M. Shara, Kenneth M. Lanzetta, Alexandra Masegian +9

Recurrent novae undergo thermonuclear-powered eruptions separated by less than 100 years, enabled by subgiant or red giant donors transferring hydrogen-rich matter at very high rat…

astro-ph.CO2024

Using HI observations of low-mass galaxies to test ultra-light axion dark matter

James T. Garland, Karen L. Masters, Daniel Grin

We evaluate recent and upcoming low-redshift neutral hydrogen (HI) surveys as a cosmological probe of small scale structure with a goal of determining the survey criteria necessary…

astro-ph.HE2023

Hydrodynamic simulations of the KT Eridani nova super-remnant

M. W. Healy-Kalesh, M. J. Darnley, M. M. Shara +3

A nova super-remnant (NSR) is an immense structure associated with a nova that forms when frequent and recurrent nova eruptions sweep up surrounding interstellar material (ISM) int…

astro-ph.GA20231 cited

Introducing the Condor Array Telescope. II. Deep imaging observations of the edge-on spiral galaxy NGC 5907 and the NGC 5866 Group: yet another view of the iconic stellar stream

Kenneth M. Lanzetta, Stefan Gromoll, Michael M. Shara +6

We used the Condor Array Telescope to obtain deep imaging observations through the luminance filter of the entirety of the NGC 5866 Group, including a very extended region surround…

astro-ph.GA2023

HI Rich but Low Star Formation galaxies in MaNGA: Physical Properties and Comparison to Control Samples

Anubhav Sharma, Karen L. Masters, David V. Stark +4

Gas rich galaxies are typically star-forming. We make use of HI-MaNGA, a program of HI follow-up for the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey of the S…

astro-ph.SR2023

Speckle Imaging of Gamma2 Velorum: The Inner Wind Possibly Resolved

Michael M. Shara, Steve B. Howell, Elise Furlan +3

Accurately quantifying the rates dM/dt at which massive stars lose mass is essential to any understanding of their evolution. All dM/dt estimates to date assume wind clumping facto…