399 citations · 1.8k across the 40 of their papers we have counts for
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Probing the All-sky Distribution of Soft X-ray Emission Associated with the Milky Way
Kazuki Ampuku, Ikuyuki Mitsuishi, Philip Kaaret +5
We present an all-sky analysis of soft X-ray emission associated with the Milky Way using HaloSat and ROSAT data, extending our previous study of five Galactic-plane regions to 330…
Widespread Detection of Two Components in the Hot Circumgalactic Medium of the Milky Way
Jesse Bluem, Philip Kaaret, K. D. Kuntz +6
Surrounding the Milky Way (MW) is the circumgalactic medium (CGM), an extended reservoir of hot gas that has significant implications for the evolution of the MW. We used the HaloS…
Optical Identification and Spectroscopy of Supernova Remnants in the Galaxy M51
P. Frank Winkler, Sadie C. Coffin, William P. Blair +2
Using a combination of ground-based and HST imaging, we have constructed a catalog of 179 supernova remnants (SNRs) and SNR candidates in the nearby spiral galaxy M51. Follow-up sp…
A disk-dominated and clumpy circumgalactic medium of the Milky Way seen in X-ray emission
P. Kaaret, D. Koutroumpa, K. D. Kuntz +7
The Milky Way galaxy is surrounded by a circumgalactic medium (CGM) that may play a key role in galaxy evolution as the source of gas for star formation and a repository of metals…
A Hard X-ray Study of the Normal Star-Forming Galaxy M83 with NuSTAR
M. Yukita, A. E. Hornschemeier, B. D. Lehmer +19
We present results from sensitive, multi-epoch NuSTAR observations of the late-type star-forming galaxy M83 (d=4.6 Mpc), which is the first investigation to spatially resolve the h…
A Deep Chandra ACIS Survey of M83
Knox S. Long, Kip D. Kuntz, William P. Blair +5
We have obtained a series of deep X-ray images of the nearby galaxy M83 using Chandra, with a total exposure of 729 ks. Combining the new data with earlier archival observations to…
The Chandra ACIS Survey of M33: X-ray, Optical and Radio Properties of the Supernova Remnants
Knox S. Long, William P. Blair, P. Frank Winkler +13
M33 contains a large number of emission nebulae identified as supernova remnants (SNRs) based on the high [S II]:Ha ratios characteristic of shocked gas. Using Chandra data from th…