Fayl:Accretion disk.jpg

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English: Artist's rendition of a black hole with an orbiting companion star that overflows its Roche lobe. Mass from the companion star is drawn towards the black hole, forming an accretion disk. GRO J1655-40 is the second so-called 'microquasar' discovered in our Galaxy. Microquasars are black holes of about the same mass as a star. They behave as scaled-down versions of much more massive black holes that are at the cores of extremely active galaxies, called quasars. Astronomers have known about the existence of stellar-mass black holes since the early 1970s. Their masses can range from 3.5 to approximately 15 times the mass of our Sun. Using Hubble data, astronomers were able to describe the black-hole system. The companion star had apparently survived the original supernova explosion that created the black hole. It is an aging star that completes an orbit around the black hole every 2.6 days. It is being slowly devoured by the black hole. Blowtorch-like jets (shown in blue) are streaming away from the black-hole system at 90 percent of the speed of light.
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Mənbə https://hubblesite.org/contents/media/images/2002/30/1273-Image.html
Müəllif ESA, NASA, and Felix Mirabel (French Atomic Energy Commission and Institute for Astronomy and Space Physics/Conicet of Argentina)

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This file is licensed under the Creative Commons Attribution 4.0 International license.
İstinad: ESA/Hubble
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Aşağıdakı şərtlərə riayət etməklə:
  • istinad – Müvafiq kredit verməlisiniz, lisenziyaya bir keçid verməlisiniz və dəyişikliklərin olub olmadığını bildirməlisiniz. Bunu hər hansı bir ağlabatan şəkildə edə bilərsiniz, ancaq lisenziyalaşdırıcının sizi və ya istifadənizi təsdiqləməsini təklif edən bir şəkildə deyil.
This file, which was originally posted to Hubble Site, was reviewed on 17 May 2020 by reviewer Green Giant, who confirmed that it was available there under the stated license on that date.

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Artist's View of Black Hole and Companion Star GRO J1655-40

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18 noyabr 2002

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indiki15:17, 26 aprel 201915:17, 26 aprel 2019 tarixindəki versiyanın kiçildilmiş görüntüsü3.000 × 2.400 (679 KB)FriedrichKiefererBetter quality.
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