Search Publications

Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1
DOI: 10.1126/science.add5399 Bibcode: 2022Sci...378..650K

Ingram, Adam; Wu, Kinwah; Enoto, Teruaki +111 more

A black hole x-ray binary (XRB) system forms when gas is stripped from a normal star and accretes onto a black hole, which heats the gas sufficiently to emit x-rays. We report a polarimetric observation of the XRB Cygnus X-1 using the Imaging X-ray Polarimetry Explorer. The electric field position angle aligns with the outflowing jet, indicating t…

2022 Science
Gaia INTEGRAL 121
A transient radio source consistent with a merger-triggered core collapse supernova
DOI: 10.1126/science.abg6037 Bibcode: 2021Sci...373.1125D

Kulkarni, S. R.; Hallinan, G.; Horesh, A. +10 more

A core collapse supernova occurs when exothermic fusion ceases in the core of a massive star, which is typically caused by exhaustion of nuclear fuel. Theory predicts that fusion could be interrupted earlier by merging of the star with a compact binary companion. We report a luminous radio transient, VT J121001+495647, found in the Very Large Arra…

2021 Science
INTEGRAL eHST 34
A fast and long-lived outflow from the supermassive black hole in NGC 5548
DOI: 10.1126/science.1253787 Bibcode: 2014Sci...345...64K

Kaastra, J. S.; Harrison, F. A.; Nandra, K. +31 more

Supermassive black holes in the nuclei of active galaxies expel large amounts of matter through powerful winds of ionized gas. The archetypal active galaxy NGC 5548 has been studied for decades, and high-resolution x-ray and ultraviolet (UV) observations have previously shown a persistent ionized outflow. An observing campaign in 2013 with six spa…

2014 Science
INTEGRAL XMM-Newton eHST 197
Early 56Ni decay gamma rays from SN2014J suggest an unusual explosion
DOI: 10.1126/science.1254738 Bibcode: 2014Sci...345.1162D

Diehl, Roland; Grebenev, Sergei A.; Greiner, Jochen +7 more

Type Ia supernovae result from binary systems that include a carbon-oxygen white dwarf, and these thermonuclear explosions typically produce 0.5 solar mass of radioactive 56Ni. The 56Ni is commonly believed to be buried deeply in the expanding supernova cloud. In SN2014J, we detected the lines at 158 and 812 kiloelectron volt…

2014 Science
INTEGRAL 104
Polarized Gamma-Ray Emission from the Galactic Black Hole Cygnus X-1
DOI: 10.1126/science.1200848 Bibcode: 2011Sci...332..438L

Rodriguez, J.; Wilms, J.; Laurent, P. +3 more

Because of their inherently high flux allowing the detection of clear signals, black hole x-ray binaries are interesting candidates for polarization studies, even if no polarization signals have been observed from them before. Such measurements would provide further detailed insight into these sources’ emission mechanisms. We measured the polariza…

2011 Science
INTEGRAL 197
Polarized Gamma-Ray Emission from the Crab
DOI: 10.1126/science.1149056 Bibcode: 2008Sci...321.1183D

Hill, A. B.; Bird, A. J.; Ubertini, P. +7 more

Pulsar systems accelerate particles to immense energies. The detailed functioning of these engines is still poorly understood, but polarization measurements of high-energy radiation may allow us to locate where the particles are accelerated. We have detected polarized gamma rays from the vicinity of the Crab pulsar using data from the spectrometer…

2008 Science
INTEGRAL 167