activity
20162024
most citedULX spectra revisited: Accreting, highly magnetized neutron stars as the engines of ultraluminous X-ray sources

95 citations · 562 across the 27 of their papers we have counts for

collaborators
Showing 2018Show all

5 papers · 1 filter

astro-ph.HE2018

NGC 300 ULX1: A test case for accretion torque theory

Georgios Vasilopoulos, Frank Haberl, Stefania Carpano +1

NGC 300 ULX1 is a newly identified ultra-luminous X-ray pulsar. The system is associated with the supernova impostor SN 2010da that was later classified as a possible supergiant Be…

astro-ph.HE2018

Investigating ULX accretion flows and cyclotron resonance in NGC 300 ULX1

Filippos Koliopanos, Georgios Vasilopoulos, Johannes Buchner +2

Methods. We analyzed broadband XMM-Newton and NuSTAR observations of NGC 300 ULX1, performing phase-averaged and phase-resolved spectroscopy. We compared two physically motivated m…

astro-ph.HE2018

NGC 300 ULX1: A new ULX pulsar in NGC 300

Chandreyee Maitra, Stefania Carpano, Frank Haberl +1

NGC 300 ULX1 is the fourth to be discovered in the class of the ultra-luminous X-ray pulsars. Pulsations from NGC 300 ULX1 were discovered during simultaneous XMM-Newton / NuSTAR o…

astro-ph.SR2018

Resolving the kinematics of the disks around Galactic B[e] supergiants

Grigoris Maravelias, Michaela Kraus, Lydia S. Cidale +4

B[e] Supergiants are luminous evolved massive stars. The mass-loss during this phase creates a complex circumstellar environment with atomic, molecular, and dusty regions usually f…

astro-ph.HE2018

Discovery of pulsations from NGC 300 ULX1 and its fast period evolution

S. Carpano, F. Haberl, C. Maitra +1

The supernova impostor SN 2010da located in the nearby galaxy NGC 300, later identified as a likely supergiant B[e] high-mass X-ray binary, was simultaneously observed by NuSTAR an…