<\/p>\n\n\n\n
![\"\"](\"https:\/\/kosmos-os.de\/wp-content\/uploads\/2025\/05\/LRGB02-paintnet-ausschn-1024x659.jpg\")
Links neben dem Quasar ist die Galaxie UGC 7604, die von der Seite zu sehen ist, schwach zu erkennen. Mit einer Rotverschiebung von z = 0,023 <\/em>[4] und daraus berechneter Lichtlaufzeit von ca. 300 Mio. Jahren <\/em>[5] ist sie im Vergleich zu TON 618 schon fast unser \u201eNachbar\u201c.<\/em><\/em><\/em><\/figcaption><\/figure>\n\n\n\n
* ___________________________________________________________<\/p>\n\n\n\n [1] O. Shemmer et al, THE ASTROPHYSICAL JOURNAL, 614:???\u2013???, 2004 OCTOBER 10, https:\/\/arxiv.org\/pdf\/astro-ph\/0406559<\/a> On April 26, 2025, I took a photograph showing an area on the border between the constellation Canes Venatici and the constellation Coma Berenices. It's probably the most unspectacular photograph I've ever taken. However, among the recognizable stars and objects is my personal record holder.<\/p>","protected":false},"author":2,"featured_media":6412,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_eb_attr":"","footnotes":""},"categories":[183],"tags":[135],"class_list":["post-6414","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-quasare","tag-quasar"],"_links":{"self":[{"href":"https:\/\/kosmos-os.de\/en\/wp-json\/wp\/v2\/posts\/6414","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/kosmos-os.de\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/kosmos-os.de\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/kosmos-os.de\/en\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/kosmos-os.de\/en\/wp-json\/wp\/v2\/comments?post=6414"}],"version-history":[{"count":3,"href":"https:\/\/kosmos-os.de\/en\/wp-json\/wp\/v2\/posts\/6414\/revisions"}],"predecessor-version":[{"id":6417,"href":"https:\/\/kosmos-os.de\/en\/wp-json\/wp\/v2\/posts\/6414\/revisions\/6417"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/kosmos-os.de\/en\/wp-json\/wp\/v2\/media\/6412"}],"wp:attachment":[{"href":"https:\/\/kosmos-os.de\/en\/wp-json\/wp\/v2\/media?parent=6414"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/kosmos-os.de\/en\/wp-json\/wp\/v2\/categories?post=6414"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/kosmos-os.de\/en\/wp-json\/wp\/v2\/tags?post=6414"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}
<\/p>\n\n\n\n![\"\"](\"https:\/\/kosmos-os.de\/wp-content\/uploads\/2025\/05\/Position-von-TON-618-1024x592.png\")
Rektaszension 12h 28m 25s | Deklination +31\u00b0 28\u2032 38\u2033
Quelle: Stellarium<\/em><\/figcaption><\/figure>\n\n\n\n
___________________________________________________________<\/p>\n\n\n\n
Der sog. Dopplereffekt bewirkt, dass das Licht, das von einem bewegten Objekt ausgesendet wird, in seiner Wellenl\u00e4nge ver\u00e4ndert ist. Kommt das Objekt auf uns zu, ist die Wellenl\u00e4nge verk\u00fcrzt, entfernt es sich von uns, ist die Wellenl\u00e4nge vergr\u00f6\u00dfert. In der sog. Akkretionsscheibe eines Quasars gibt es in dem turbulenten Gas beide F\u00e4lle, so dass die jeweiligen Emissionslinien der verschiedenen Gase aufgeweitet erscheinen.<\/p>\n\n\n\n
[2] NASA\/IPAC Extragalactic Database, https:\/\/ned.ipac.caltech.edu\/cgi-bin\/nph-objsearch?objname=RX%20J1228.4%2B3128&extend=no&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES<\/a>
[3] https:\/\/www.guinnessworldrecords.com\/world-records\/76251-heaviest-black-hole?utm_source=chatgpt.com<\/a>
[4]https:\/\/simbad.u-strasbg.fr\/simbad\/sim-id?Ident=UGC+7604&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id<\/a>
[5] https:\/\/astro.goblack.de\/Theorie\/t_tools.html<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"