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^[1] The Cloverleaf Quasar is a gravitational-ally lensed quasar which contains a substantial dust content. This also infers that the quasar contains a large amount of gas as well. The gravitational field of at least one if not more foreground galaxies was bent in such a way that it magnified the light from the quasar to produce more than one image. This magnification can be the result of the X-rays in this quasar coming from a small section of its black hole and the optical light comes from a different area. This phenomenon of bending light in order to detect astronomical objects is called gravitational microlensing ^[2] AjBongiorno (talk) 16:19, 5 December 2016 (UTC)

^ Barvainis, R., Antonucci, R. & Coleman, P. Astrophys. J. 399, L19−L22 (1992). {{cite web}}: Missing or empty |title= (help); Missing or empty |url= (help)CS1 maint: multiple names: authors list (link) CS1 maint: numeric names: authors list (link)
^ G. Chartas et al. 2004 Astrophys. J. 606, 78. {{cite web}}: Missing or empty |title= (help); Missing or empty |url= (help)CS1 maint: numeric names: authors list (link)

[1] Barvainis, R., Antonucci, R. & Coleman, P. Astrophys. J. 399, L19−L22 (1992). {{cite web}}: Missing or empty |title= (help); Missing or empty |url= (help)CS1 maint: multiple names: authors list (link) CS1 maint: numeric names: authors list (link)

[2] G. Chartas et al. 2004 Astrophys. J. 606, 78. {{cite web}}: Missing or empty |title= (help); Missing or empty |url= (help)CS1 maint: numeric names: authors list (link)

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Revision as of 16:19, 5 December 2016 edit AjBongiorno (talk \| contribs) 6 edits mNo edit summary Tag: Visual edit: Switched ← Previous edit		Latest revision as of 16:19, 5 December 2016 edit undo AjBongiorno (talk \| contribs) 6 edits No edit summary Tag: Visual edit
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	<ref>{{cite web\|last1=Barvainis, R., Antonucci, R. & Coleman, P. Astrophys. J. 399, L19−L22 (1992)}}</ref>		<ref>{{cite web\|last1=Barvainis, R., Antonucci, R. & Coleman, P. Astrophys. J. 399, L19−L22 (1992)}}</ref>
	The Cloverleaf is a gravitational-ally lensed quasar which contains a substantial dust content. This also infers that the quasar contains a large amount of gas as well. The gravitational field of at least one if not more foreground galaxies was bent in such a way that it magnified the light from the quasar to produce more than one image. This magnification can be the result of the X-rays in this quasar coming from a small section of its black hole and the optical light comes from a different area. This phenomenon of bending light in order to detect astronomical objects is called gravitational microlensing <ref>{{cite web\|last1=G. Chartas et al. 2004 Astrophys. J. 606, 78}}</ref> [[User:AjBongiorno\|AjBongiorno]] ([[User talk:AjBongiorno\|talk]]) 16:19, 5 December 2016 (UTC)		The Cloverleaf Quasar is a gravitational-ally lensed quasar which contains a substantial dust content. This also infers that the quasar contains a large amount of gas as well. The gravitational field of at least one if not more foreground galaxies was bent in such a way that it magnified the light from the quasar to produce more than one image. This magnification can be the result of the X-rays in this quasar coming from a small section of its black hole and the optical light comes from a different area. This phenomenon of bending light in order to detect astronomical objects is called gravitational microlensing <ref>{{cite web\|last1=G. Chartas et al. 2004 Astrophys. J. 606, 78}}</ref> [[User:AjBongiorno\|AjBongiorno]] ([[User talk:AjBongiorno\|talk]]) 16:19, 5 December 2016 (UTC)