papers

Publications (11)

astro-ph.HE2016

Evidence for simultaneous jets and disk winds in luminous low-mass X-ray binaries

Jeroen Homan, Joseph Neilsen, Jessamyn L. Allen +5

Recent work on jets and disk winds in low-mass X-ray binaries (LMXBs) suggests that they are to a large extent mutually exclusive, with jets observed in spectrally hard states and…

astro-ph2003

XMM-Newton observations of PSR B1823-13: An asymmetric synchrotron nebula around a Vela-like pulsar

Bryan Gaensler, Norbert Schulz, Vicky Kaspi +2

We present a deep observation with the X-ray Multi-Mirror Mission of PSR B1823-13, a young pulsar with similar properties to the Vela pulsar. We detect two components to the X-ray…

astro-ph.HE2024

Revealing the state transition of Cen X-3 at high spectral resolution with Chandra

Graciela Sanjurjo-Ferrín, Jose Miguel Torrejón, Lida Oskinova +4

Cen X-3 is a compact, high-mass X-ray binary (HMXRB), likely powered by Roche lobe overflow. We present a phase-resolved X-ray spectral and timing analysis of a target of opportuni…

astro-ph.EP2019

Astro 2020: Astromineralogy of interstellar dust with X-ray spectroscopy

Lia Corrales, Lynne Valencic, Elisa Costantini +16

X-ray absorption fine structure (XAFS) in the 0.2-2 keV band is a crucial component in multi-wavelength studies of dust mineralogy, size, and shape -- parameters that are necessary…

astro-ph2006

Chandra Detection of Fe XVII in Absorption: Iron Abundance in the Hot Gaseous Interstellar Medium

Yangsen Yao, Norbert Schulz, Q. Daniel Wang +1

The iron depletion level and the gas-phase iron abundance in the hot ~10^6 K interstellar medium (ISM) is critical to the understanding of its energy balance as well as the thermal…

astro-ph2006

Star Formation in the Era of the Three Great Observatories

Scott J. Wolk, Norbert Schulz, John Stauffer +6

This paper summarizes contributions and suggestions as presented at the Chandra Workshop Star Formation in the Era of Three Great Observatories conducted in July 2005. One of the d…

astro-ph.HE2011

Suzaku Observations of 4U 1957+11: Potentially the Most Rapidly Spinning Black Hole in (the Halo of) the Galaxy

Michael A. Nowak, Joern Wilms, Katja Pottschmidt +3

We present three Suzaku observations of the black hole candidate 4U 1957+11 (V1408 Aql) --- a source that exhibits some of the simplest and cleanest examples of soft, disk-dominate…

astro-ph.HE2025

Cyclical accretion regime change in the slow X-ray pulsar 4U 0114+65 observed with Chandra

Graciela Sanjurjo-Ferrín, Jose Miguel Torrejón, Konstantin Postnov +5

4U 0114+65 is a high-mass X-ray binary system formed by the luminous supergiant B1Ia, known as V{*} V662 Cas, and one of the slowest rotating neutron stars (NS) with a spin period…

astro-ph.IM2009

Broad-Band Soft X-ray Polarimetry

Herman L. Marshall, Ralf Heilmann, Norbert Schulz +1

We developed an instrument design capable of measuring linear X-ray polarization over a broad-band using conventional spectroscopic optics. A set of multilayer-coated flats reflect…

astro-ph.HE2025

A persistent disk wind and variable jet outflow in the neutron-star low-mass X-ray binary GX 13+1

Daniele Rogantini, Jeroen Homan, Richard M. Plotkin +6

In low-mass X-ray binaries (LMXBs), accretion flows are often associated with either jet outflows or disk winds. Studies of LMXBs with luminosities up to roughly 20% of the Eddingt…

astro-ph.HE2025

Connecting dust and outflows in AGN: the intriguing case of NGC 6860

Ioanna Psaradaki, Missagh Mehdipour, Daniele Rogantini +4

Cosmic dust plays a crucial role in the evolution of galaxies, significantly influencing star formation and the interstellar medium. However, in active galactic nuclei (AGN), the r…