activity
20002017
most citedSolar abundance ratios of the iron-peak elements in the Perseus Cluster

116 citations · 212 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2017★ 116 cited

Solar abundance ratios of the iron-peak elements in the Perseus Cluster

Hitomi Collaboration

The metal abundance of the hot plasma that permeates galaxy clusters represents the accumulation of heavy elements produced by billions of supernovae. Therefore, X-ray spectroscopy…

astro-ph.GA2011

Implications of the SPEAR FUV Maps on Our Understanding of the ISM

Eric J. Korpela, Martin Sirk, Jerry Edelstein +3

The distribution of a low-density transition temperature (10^4.5 - 10^5.5 K) gas in the interstellar medium conveys the character and evolution of diffuse matter in the Galaxy. Thi…

astro-ph2008★ 4 cited

Modeling the Local Warm/Hot Bubble

Dieter Breitschwerdt, Miguel A. de Avillez, Verena Baumgartner

In this paper we review the modeling of the Local Bubble (LB) with special emphasis on the progress we have made since the last major conference "The Local Bubble and Beyond (I)" h…

astro-ph2001★ 28 cited

A New ASCA and ROSAT Study of the Supernova Remnant: G272.2-3.2

I. M. Harrus, P. O. Slane, R. Smith +1

G272.2-3.2 is a supernova remnant (SNR) characterized by an apparent centrally brightened X-ray morphology and thermally dominated X-ray emission. Because of this combination of Se…

astro-ph2000★ 64 cited

Chandra X-ray Observatory Arcsecond Imaging of the Young, Oxygen-rich Supernova Remnant 1E0102.2-7219

T. J. Gaetz, Yousaf M. Butt, Richard J. Edgar +4

We present observations of the young, Oxygen-rich supernova remnant 1E0102.2-7219 taken by the Chandra X-ray Observatory during Chandra's Orbital Activation and Checkout phase. The…