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20002025
most citedThe Chandra HETGS and RXTE view of GRS 1915+105

200 citations · 1.1k across the 21 of their papers we have counts for

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astro-ph.HE2025★ 3 cited

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.HE2024★ 7 cited

A Time-Dependent Spectral Analysis of Cassiopeiae

Sean J. Gunderson, David P. Huenemoerder, José M. Torrejón +7

We investigated the temporal and spectral features of Cassiopeiae's X-ray emission within the context of the white dwarf accretion hypothesis. We find that the variabilities pr…

astro-ph.HE2024★ 5 cited

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.HE2017★ 48 cited

The clumpy absorber in the high-mass X-ray binary Vela X-1

V. Grinberg, N. Hell, I. El Mellah +13

Bright and eclipsing, the high-mass X-ray binary Vela X-1 offers a unique opportunity to study accretion onto a neutron star from clumpy winds of O/B stars and to disentangle the c…

astro-ph.HE2012★ 19 cited

Chandra and Suzaku observations of the Be/X-ray star HD110432

Jose M. Torrejon, Norbert S. Schulz, Michael A. Nowak

We present an analysis of a pointed 141 ks Chandra high resolution transmission gratings observation of the Be X-ray emitting star HD110432, a prominent member of the gamma Cas ana…

astro-ph.HE2010★ 16 cited

Dynamical Ne K Edge and Line Variations in the X-Ray Spectrum of the Ultra-compact Binary 4U 0614+091

Norbert S. Schulz, Michael P. Nowak, Deepto Chakrabarty +1

We observed the ultra-compact binary candidate 4U 0614+091 for a total of 200 ksec with the high-energy transmission gratings onboard the \chandra X-ray Observatory. The source is…