Co je ngc 1277

Tato funkce je na stránkách Astronomia nová a texty zatím nejsou označené obtížností Testy. Zvolte oblast, ze které chcete otestovat Data pro NGC Nov 29, 2012 · The lenticular galaxy NGC 1277 lies about 220 million light-years away in the constellation Perseus. It is only ten percent the size and mass of our Milky Way Galaxy. It is only ten percent the ngc 1277 е леќеста галаксија во соѕвездието Персеј, која се наоѓа на списокот на Новиот општ каталог на објекти на длабокото небо. We report the detection of CO(1-0) emission from NGC 1277, a lenticular galaxy in the Perseus Cluster.

13.10.2020 Co je ngc 1277

[1] Query : NGC 1277 C.D.S. - SIMBAD4 rel 1.7 - 2021.02.23CET07:25:44 Available data : Basic data • Identifiers • Plot & images • Bibliography • Measurements • External archives • Notes • Annotations NGC 1277 là một thiên hà hình hạt đậu trong chòm sao Anh Tiên. Nó là một thành viên của cụm Perseus và nằm khoảng 73Mpc (Mega parsec) hay 220 triệu năm ánh sáng từ Ngân Hà. Nó có cấp sao biểu kiến là khoảng 14,7. NGC 1277 je čočková galaxie v souhvězdí Persea vzdálená přibližně 186 milionů světelných let od Mléčné dráhy.Je členem Kupy galaxií v Perseovi.Její hvězdná velikost je 13,7.

25/08/2019

This galaxy shines at apparent … NGC-1277- 0 points 1 point 2 points 2 months ago * Taken with a Sony a6000 I’m still learning all the settings and need to purchase a lens that has a lower aperture (currently this is … NGC 1277. Idi na navigaciju Idi na pretragu. NGC 1277.

We report the detection of CO(1-0) emission from NGC 1277, a lenticular galaxy in the Perseus Cluster. NGC 1277 has previously been proposed to host an overmassive black hole (BH) compared to the

Dutch astronomer Remco van den Bosch and co-workers weighed the black hole at the center of this galaxy. The percentage ofidentified S+Irr increases, however, increases from 30% in the centre tomore than 50% in the outer parts. The projected distributions of early-and late-type galaxies are not co-centred. The total luminosity of allsupposed member galaxies in the surveyed area is estimated to(6.5+/-0.9)\ 10(12) x h50(-2) blue solar luminosities. According to van den Bosch and his co-authors, NGC 1277 resembles a class of highly compact, rotating, and massive "red, passive galaxies" that existed as far back as 10 billion years ago, with Here we provide our measurements for NGC 1277. Our structural decomposition reveals that NGC 1277 is dominated by a “classical” spheroid with a Sérsic index n = 5.3, a half-light radius R e,major =2.1 kpc, and a stellar mass of 2.7 10´ 11 M (using ML* V =11.65, Martín-Navarro et al.).Thismassis
All rights reserved. Un des plus grands problèmes cependant, est que NGC1277 est une galaxie lenticulaire, un type de galaxies qui possèdent généralement Tato funkce je na stránkách Astronomia nová a texty zatím nejsou označené obtížností Testy.

Pogledajte NGC 1277. Product/Service. See more of NGC 1277 on Facebook.

It is a member of the Perseus Cluster of galaxies and is located approximately 220 million light years from the Milky Way. It has a visual magnitude of 14.7. It was discovered on December 4, 1875 by Lawrence Parsons, 4th Earl of Rosse. Ancient stars NGC 1277 Súradnice: 03h 19m 51s; 41° 34′ 27″ NGC 1277 je galaxia v súhvezdí Perzeus, ktorú objavil írsky astronóm Lawrence Parsons 4. decembra 1875. Jej zdanlivá hviezdna veľkosť je 13,8. Mar 12, 2018 · At some point, NGC 1277 stopped producing stars, and the aging ones became reddish lights that Hubble could spot.

NGC 1277 is moving so fast through the cluster, at 2 million miles (3.2 million km) per hour, that it cannot ngc 1277 (іншыя абазначэнні — mcg 7-7-64, zwg 540.104, pgc 12434) — кампактная лінзападобная галактыка ў сузор’і Персей. Гэты аб’ект уваходзіць у лік пералічаных у арыгінальнай рэдакцыі « Новага агульнага Here we provide our measurements for NGC 1277. Our structural decomposition reveals that NGC 1277 is dominated by a “classical” spheroid with a Sérsic index n = 5.3, a half-light radius R e,major =2.1 kpc, and a stellar mass of 2.7 10´ 11 M (using ML* V =11.65, Martín-Navarro et al.).Thismassis NGC 1276 je dvojhviezda v súhvezdí Perzeus, ktorú objavil dánsko-írsky astronóm John Dreyer 12. decembra 1876. … | NGC 1275 | NGC 1276 | NGC 1277 | … Tento článok týkajúci sa deep sky objektov je zatiaľ „ výhonok “. ngc 1277 нысанына арналған жарияланымдар Бұл — Галактика туралы мақаланың бастамасы . Бұл мақаланы толықтырып, дамыту арқылы, Уикипедияға көмектесе аласыз.

decembra 1876. … | NGC 1275 | NGC 1276 | NGC 1277 | … Tento článok týkajúci sa deep sky objektov je zatiaľ „ výhonok “. ngc 1277 нысанына арналған жарияланымдар Бұл — Галактика туралы мақаланың бастамасы . Бұл мақаланы толықтырып, дамыту арқылы, Уикипедияға көмектесе аласыз. NGC 1277 bývá nazývána jako "pozůstatek raného vesmíru", protože se její hvězdy tvořily během 100 miliónů let dlouhého období před více než dvanácti miliardami let, když byl vesmír starý pouze 2 miliardy let. NGC 1277 is a lenticular galaxy in the constellation of Perseus. It is a member of the Perseus Cluster of galaxies and is located approximately 73 Mpc (megaparsecs) or 220 million light years from the Milky Way. It has an apparent magnitude of about 14.7.

NGC 1277 je još poznat i pod oznakama MCG 7-7-64, CGCG 540-104, PGC 12434. NGC 1277 je galaksija u zviježđu Perzej. The percentage ofidentified S+Irr increases, however, increases from 30% in the centre tomore than 50% in the outer parts. The projected distributions of early-and late-type galaxies are not co-centred. The total luminosity of allsupposed member galaxies in the surveyed area is estimated to(6.5+/-0.9)\ 10(12) x h50(-2) blue solar luminosities. NGC 1277 is a lenticular galaxy located in Perseus constellation. It lies at a distance of about 220 million light years from Earth.

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NGC 1277 је лентикуларна галаксија у сазвежђу Персеј која се налази на NGC листи објеката дубоког неба.. Деклинација објекта је + 41° 34' 27" а ректасцензија 3h 19m 51,4s. Привидна величина (магнитуда) објекта NGC 1277 износи 13,8 а

NGC 1277 is a lenticular galaxy in the constellation of Perseus. It is a member of the Perseus Cluster of galaxies and is located approximately 73 Mpc (megaparsecs) or 220 million light years from the Milky Way. It has an apparent magnitude of about 14.7. It was discovered on December 4, 1875 by Lawrence Parsons, 4th Earl of Rosse. NGC 1277 (također poznat kao MCG 7-7-64 i PGC 12434) je spiralna galaksija koja je udaljena oko 233 miliona sg od Zemlje i nalazi se u sazviježđu Perzej. Najveći prečnik je 0,80 (54 hiljade sg) a najmanji 0,3 uglovnih minuta (20 hiljada sg). Prvo otkriće je napravio Lawrence, 4.