activity
20082026
most citedFirst Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

1.9k citations · 8k across the 194 of their papers we have counts for

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Showing 2012Show all

13 papers · 1 filter

astro-ph.HE2012★ 67 cited

X-ray emission and absorption features during an energetic thermonuclear X-ray burst from IGR J17062-6143

N. Degenaar, J. M. Miller, R. Wijnands +2

Type-I X-ray bursts are thermonuclear explosions occurring in the surface layers of accreting neutron stars. These events are powerful probes of the physics of neutron stars and th…

astro-ph.HE2012★ 45 cited

A direct measurement of the heat release in the outer crust of the transiently accreting neutron star XTE J1709-267

N. Degenaar, R. Wijnands, J. M. Miller

The heating and cooling of transiently accreting neutron stars provides a powerful probe of the structure and composition of their crust. Observations of superbursts and crust cool…

astro-ph.HE2012★ 1 cited

The transient neutron star X-ray binary KS 1741-293 in outburst and quiescence

N. Degenaar, R. Wijnands

KS 1741-293 is a transient neutron star low-mass X-ray binary that is located at an angular distance of ~20' from the Galactic center. We map out the historic activity of the sourc…

astro-ph.HE2012★ 1 cited

A peculiar thermonuclear X-ray burst from the transiently accreting neutron star SAX J1810.8-2609

N. Degenaar, R. Wijnands

We report on a thermonuclear (type-I) X-ray burst that was detected from the neutron star low-mass X-ray binary SAX J1810.8-2609 in 2007 with Swift. This event was longer (~20 min)…

astro-ph.HE2012★ 60 cited

The X-ray flaring properties of Sgr A* during six years of monitoring with Swift

N. Degenaar, J. M. Miller, J. Kennea +2

Starting in 2006, Swift has been targeting a region of ~21'X21' around Sagittarius A* (Sgr A*) with the onboard X-ray telescope. The short, quasi-daily observations offer an unique…

astro-ph.HE2012★ 77 cited

Testing the deep-crustal heating model using quiescent neutron-star very-faint X-ray transients and the possibility of partially accreted crusts in accreting neutron stars

Rudy Wijnands, Nathalie Degenaar, Dany Page

It is assumed that accreting neutron stars (NSs) in LMXBs are heated due to the compression of the existing crust by the accreted matter which gives rise to nuclear reactions in th…