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Bright black holes and neutron stars beat alike
by
Motta, Sara Elisa
, Kalemci, Emrah
in
Accretion disks
/ Arrays
/ Astronomy
/ Binary stars
/ Black holes
/ Deposition
/ Emission analysis
/ European Southern Observatory
/ Hubble Space Telescope
/ Neutron radiation
/ Neutron stars
/ Neutrons
/ Observatories
/ Radiation
/ Radio signals
/ Space telescopes
/ Spectroscopic telescopes
/ Stars
/ Stars & galaxies
/ Ultraviolet astronomy
/ Very Large Telescope
/ Wavelength
/ X-ray astronomy
/ X-rays
2023
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Bright black holes and neutron stars beat alike
by
Motta, Sara Elisa
, Kalemci, Emrah
in
Accretion disks
/ Arrays
/ Astronomy
/ Binary stars
/ Black holes
/ Deposition
/ Emission analysis
/ European Southern Observatory
/ Hubble Space Telescope
/ Neutron radiation
/ Neutron stars
/ Neutrons
/ Observatories
/ Radiation
/ Radio signals
/ Space telescopes
/ Spectroscopic telescopes
/ Stars
/ Stars & galaxies
/ Ultraviolet astronomy
/ Very Large Telescope
/ Wavelength
/ X-ray astronomy
/ X-rays
2023
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Do you wish to request the book?
Bright black holes and neutron stars beat alike
by
Motta, Sara Elisa
, Kalemci, Emrah
in
Accretion disks
/ Arrays
/ Astronomy
/ Binary stars
/ Black holes
/ Deposition
/ Emission analysis
/ European Southern Observatory
/ Hubble Space Telescope
/ Neutron radiation
/ Neutron stars
/ Neutrons
/ Observatories
/ Radiation
/ Radio signals
/ Space telescopes
/ Spectroscopic telescopes
/ Stars
/ Stars & galaxies
/ Ultraviolet astronomy
/ Very Large Telescope
/ Wavelength
/ X-ray astronomy
/ X-rays
2023
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Journal Article
Bright black holes and neutron stars beat alike
2023
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Overview
Astronomy Multi-wavelength observations of radiation from a bright neutron-star system show signatures similar to that of a black-hole binary, suggesting that the accretion mechanism is the same for all such sources at high luminosities. [...]previous studies reported emission characterized by flashes of light from the neutron star's surface6, variability patterns that resemble those of GRS 915+105, and outflows in X-ray, optical and ultraviolet frequencies7 - the X-ray signals suggesting the presence of material near the neutron star2. NASA's Nuclear Spectroscopic Telescope Array was used to obtain high-resolution X-ray signals; the Hubble Space Telescope accessed ultraviolet frequencies; the Liverpool Telescope in Spain was used for optical frequencies; the European Southern Observatory's Very Large Telescope in Chile covered the near infrared; and the Karl G.Jansky Very Large Array in New Mexico observed radio-wavelength signals.
Publisher
Nature Publishing Group
Subject
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