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İzahAccretion disk.jpg
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.
ESA, NASA, and Felix Mirabel (French Atomic Energy Commission and Institute for Astronomy and Space Physics/Conicet of Argentina)
Lisenziya
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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.
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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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Fayl Faylin tarixcesi Fayl kecidleri Faylin qlobal istifadesiSinaq gosterisi olcusu 750 600 piksel Diger olculer 300 240 piksel 600 480 piksel 960 768 piksel 1 280 1 024 piksel 2 560 2 048 piksel 3 000 2 400 piksel Faylin orijinali 8206 3 000 2 400 piksel fayl hecmi 679 KB MIME novu image jpeg Bu fayl Vikimedia Commons dadirve diger layihelerde istifade edile biler Faylin tesvir sehifesine get Xulase IzahAccretion disk jpg 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 Tarix 18 noyabr 2002 released Menbe https hubblesite org contents media images 2002 30 1273 Image html Muellif ESA NASA and Felix Mirabel French Atomic Energy Commission and Institute for Astronomy and Space Physics Conicet of Argentina Lisenziya ESA Hubble images videos and web texts are released by the ESA under the Creative Commons Attribution 4 0 International license and may on a non exclusive basis be reproduced without fee provided they are clearly and visibly credited Detailed conditions are below see the ESA copyright statement for full information For images created by NASA or on the hubblesite org website or for ESA Hubble images on the esahubble org site before 2009 use the PD Hubble tag Conditions The full image or footage credit must be presented in a clear and readable manner to all users with the wording unaltered for example ESA Hubble Web texts should be credited to ESA Hubble except when used by media The credit should not be hidden or disassociated from the image footage Links should be active if the credit is online See the usage rights Q amp A section on the ESA copyright page for guidance ESA Hubble materials may not be used to state or imply the endorsement by ESA Hubble or any ESA Hubble employee of a commercial product or service ESA Hubble requests a copy of the product sent to them to be indexed in their archive If an image shows an identifiable person using that image for commercial purposes may infringe that person s right of privacy and separate permission should be obtained from the individual If images or visuals are changed significantly from the original work apart from resizing cropping we suggest that the changes are mentioned after the credit line For example Original image by ESA Hubble M Kornmesser warping and recolouring by NN Notes Note that this general permission does not extend to the use of ESA Hubble s logo which shall remain protected and may not be used or reproduced without prior and individual written consent of ESA Hubble Also note that music scientific papers and code on the esahubble org site are not released under this license and can not be used for non ESA Hubble products By reproducing ESA Hubble material in part or in full the user acknowledges the terms on which such use is permitted This file is licensed under the Creative Commons Attribution 4 0 International license Istinad ESA HubbleAzadsiniz paylasmaq eseri kocurmek paylamaq ve oturmek ucun remiks etmek eseri adaptasiya etmek Asagidaki sertlere riayet etmekle istinad Muvafiq kredit vermelisiniz lisenziyaya bir kecid vermelisiniz ve deyisikliklerin olub olmadigini bildirmelisiniz Bunu her hansi bir aglabatan sekilde ede bilersiniz ancaq lisenziyalasdiricinin sizi ve ya istifadenizi tesdiqlemesini teklif eden bir sekilde deyil https creativecommons org licenses by 4 0 CC BY 4 0 Creative Commons Attribution 4 0 true true 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 CaptionsazerbaycancaAdd a one line explanation of what this file representsingilisArtist s View of Black Hole and Companion Star GRO J1655 40Items portrayed in this filetesvir edircopyright status nbsp ingiliscopyrighted nbsp ingilislisenziyaCreative Commons Attribution 4 0 International nbsp ingilisyaranma tarixi18 noyabr 2002 Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtKicik sekilOlculerIstifadeciSerh indiki15 17 26 aprel 20193 000 2 400 679 KB FriedrichKiefererBetter quality 23 12 15 mart 20053 000 2 400 112 KB Bebenko commonswikicopy paste from english wiki Fayl kecidleri Bu sekile olan kecidler Qara delik Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur af wikipedia org layihesinde istifadesi Swartkolk X straaldubbelster Akkresieskyf ar wikipedia org layihesinde istifadesi ثقب أسود قرص مزود بوابة علم الفلك صورة الأسبوع أرشيف تنامي GRO J1655 40 ثنائي أشعة إكس ar wikibooks org layihesinde istifadesi علم الفلك ثقوب سوداء ast wikipedia org layihesinde istifadesi Acrecimientu Stephen Hawking Teoria de la relativida Cosmos A Spacetime Odyssey Furacu negru estelar Discu d acrecimientu Binaria de Rayos X bar wikipedia org layihesinde istifadesi Schwoaz Loch bg wikipedia org layihesinde istifadesi Cherna dupka Shablon Izbrana statiya 22 Shablon Izbrana statiya 41 Uikipediya Izbrani statii Hronologiya 2005 Shablon Izbrana statiya 02 2006 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