19 Facts About X-ray astronomy

X-ray astronomy is an observational branch of astronomy which deals with the study of X-ray observation and detection from astronomical objects.

X-ray astronomy uses a type of space telescope that can see x-ray radiation which standard optical telescopes, such as the Mauna Kea Observatories, cannot.

X-ray astronomy emission is expected from astronomical objects that contain extremely hot gases at temperatures from about a million kelvin to hundreds of millions of kelvin .

The first cosmic X-ray astronomy source was discovered by a sounding rocket in 1962.

Balloon-borne experiment called the High-resolution gamma-ray and hard X-ray astronomy spectrometer observed X-ray astronomy and gamma-rays emissions from the Sun and other astronomical objects.

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X-ray astronomy telescopes have varying directionality or imaging ability based on glancing angle reflection rather than refraction or large deviation reflection.

X-ray astronomy detectors have been designed and configured primarily for energy and occasionally for wavelength detection using a variety of techniques usually limited to the technology of the time.

An intermediate-mass X-ray astronomy binary is a binary star system where one of the components is a neutron star or a black hole.

Theoretical X-ray astronomy is a branch of theoretical astronomy that deals with the theoretical astrophysics and theoretical astrochemistry of X-ray generation, emission, and detection as applied to astronomical objects.

However, the Crab Nebula appears as an X-ray astronomy source that is a central freely expanding ball of dilute plasma, where the energy content is 100 times the total energy content of the large visible and radio portion, obtained from the unknown source.

High-mass X-ray astronomy binaries are composed of OB supergiant companion stars and compact objects, usually neutron stars or black holes .

Supergiant X-ray astronomy binaries are HMXBs in which the compact objects orbit massive companions with orbital periods of a few days, and in circular orbits.

The high temperature of Capella's corona as obtained from the first coronal X-ray astronomy spectrum of Capella using HEAO 1 required magnetic confinement unless it was a free-flowing coronal wind.

However, their X-ray astronomy emission is 10 to 10 times stronger than for main-sequence stars of similar masses.

X-ray astronomy astrometry becomes a serious concern that results in ever greater demands for finer angular resolution and spectral radiance.

Soft X-ray astronomy sigmoid is an observational manifestation of the connection between coronal structure and CME production.

Altair's total X-ray astronomy luminosity is at least an order of magnitude larger than the X-ray astronomy luminosity for Vega.

X-ray astronomy observations offer the possibility to detect planets as they eclipse part of the corona of their parent star while in transit.

X-ray astronomy observations offer the possibility to detect planets as they eclipse part of the corona of their parent star while in transit.