activity
20092026
most citedAn accretion model for the anomalous X-ray pulsar 4U 0142+61

57 citations · 76 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2026

Bayesian Modeling of NICER Cometary X-ray Spectra: A Legacy Survey of Solar-Wind Charge Exchange

T. K. Deskins, Dennis Bodewits, Steven Bromley +3

We present a uniform, epoch-resolved analysis of soft X-ray observations of eight comets obtained with NICER, using Bayesian statistics to identify charge-exchange line components,…

astro-ph.SR2026★ 1 cited

Determination of the Solar System contribution to the soft X-ray sky

K. Dennerl, G. Ponti, X. Zheng +4

Solar wind charged particles interact with diffuse gas within the heliosphere, producing soft X-rays. This solar wind charge exchange (SWCX) process produces foreground emission th…

astro-ph.GA2026

Low-mass stars dominate the hot (0.7 keV) Galactic X-ray emission

G. Ponti, M. C. H. Yeung, G. Stel +12

The circumgalactic medium (CGM) of the Milky Way is composed of a tenuous atmosphere filled with multi-phase plasma, including a warm-hot virialised component. Recent studies sugge…

astro-ph.SR2025

First Resolution of a Main Sequence G-Star Astrosphere Using Chandra

C. M. Lisse, S. J. Wolk, B. Snios +24

We report resolution of a halo of X-ray line emission surrounding the Zero Age Main Sequence (ZAMS) G8.5V star HD 61005 by Chandra ACIS-S. Located only 36.4 pc distant, HD 61005 is…

astro-ph.HE2025

Searching the non-accreting white dwarf population in eROSITA data

S. Friedrich, C. Maitra, K. Dennerl +3

eROSITA is the soft X-ray instrument aboard the Spectrum Roentgen Gamma (SRG) satellite that is most sensitive in the energy range between 0.2 and 2.3 keV. Between December 2019 an…

astro-ph.HE2012★ 57 cited

An accretion model for the anomalous X-ray pulsar 4U 0142+61

J. E. Truemper, K. Dennerl, N. D. Kylafis +2

We propose that the quiescent emission of AXPs/SGRs is powered by accretion from a fallback disk, requiring magnetic dipole fields in the range 10^{12}-10^{13} G, and that the lumi…

astro-ph.HE2009★ 18 cited

Chandra's Close Encounter with the Disintegrating Comets 73P/2006 (Schwassmann--Wachmann--3) Fragment B and C/1999 S4 (LINEAR)

Scott J. Wolk, C. M. Lisse, D. Bodewits +2

On May 23, 2006 we used the ACIS-S instrument on the Chandra X-ray Observatory (CXO) to study the X-ray emission from the B fragment of comet 73P/2006 (Schwassmann-Wachmann 3) (73P…