Search Publications

X-Ray Spectroscopy in the Microcalorimeter Era. II. A New Diagnostic on Column Density from the Case A to B Transition in H- and He-like Iron
DOI: 10.3847/1538-4357/abaaac Bibcode: 2020ApJ...901...69C

Ferland, G. J.; Su, Y.; Chakraborty, P. +2 more

The Soft X-ray Spectrometer on board Hitomi, with the unprecedented resolving power of R ∼ 1250, allowed the detection of members of the Fe XXV Kα complex emission spectra from the center of the Perseus Cluster. In this paper, we introduce a novel method of measuring the column density using the optically thin (Case A) to optically thick (Case B) …

2020 The Astrophysical Journal
Hitomi 15
The Nonstandard Properties of a "Standard" PWN: Unveiling the Mysteries of PWN G21.5-0.9 Using Its IR and X-Ray Emission
DOI: 10.3847/1538-4357/abba32 Bibcode: 2020ApJ...904...32H

Gelfand, Joseph D.; Temim, Tea; Slane, Patrick O. +3 more

The evolution of a pulsar wind nebula (PWN) depends on properties of the progenitor star, supernova, and surrounding environment. As some of these quantities are difficult to measure, reproducing the observed dynamical properties and spectral energy distribution (SED) with an evolutionary model is often the best approach to estimating their values…

2020 The Astrophysical Journal
Herschel Hitomi 11