Co je ngc 1277

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. It was discovered on December 4, 1875 by Lawrence Parsons, 4th Earl of Rosse.

16.02.2021

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 galaxy bulge luminosity (mass), based on stellar-kinematic measurements. The CO(1-0) emission, observed with the IRAM Plateau de Bure Interferometer (PdBI) using both, a more compact (2.9-arcsec

godine. Jul 08, 2015 · We report the detection of CO(1-0) emission from NGC 1277, a lenticular galaxy in the Perseus Cluster.

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Ushbu obyekt Yangi umumiy katalog asl nashrida mavjud.. Qora tuynuk.

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In addition, near the galaxy cluster center, intergalactic gas is so hot it cannot cool to condense and form stars. 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 has been called a "relic of the early … Magnetic monster NGC 1275 This stunning image of NGC 1275 was taken using the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys in July and August 2006. It provides amazing detail and resolution of the fragile filamentary structures, which show up as a reddish lacy structure surrounding the central bright galaxy NGC 1275.

Ushbu obyektni Lawrence Parsons 1875-yilda kashf etgan. Ushbu obyekt Yangi umumiy katalog asl nashrida mavjud. Qora tuynuk Photometric properties of MRK 1216 and NGC 1277. (1) Morphological classification according to the NED, (2) Hubble flow distance, (3) scale at this distance, (4) effective radius in arcsec or (5) kpc, measured by a circular aperture that contains half of the light, (6) extinction corrected total luminosity of the HSTF160W (MRK 1216) and F814W (NGC 1277) exposures, (7) peak and effective Ovo je stranica za razgovor za raspravu o poboljšanjima na članku NGC 1277.; Ovo nije forum za opću raspravu o temi članka. Pisanje kojemu ovdje nije mjesto može biti premješteno ili uklonjeno. Mar 15, 2018 · Galaxy NGC 1277 lives near the center of the Perseus cluster of over 1,000 galaxies. 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.

NGC 1277 has been dubbed a “relic of the early Universe” because all of its stars appear to have formed about 12 billion years ago. To put this in perspective, the Big Bang is thought to have happened 13.8 billion years ago. Teeming with billions of old, metal-rich stars, NGC 1277 Persey yulduz turkumidagi S0-a tipli galaktikadir. Somon Yoʻlidan taqriban 220 million yorugʻlik yili uzoqlikda joylashgan.. Ushbu obyektni Lawrence Parsons 1875-yilda kashf etgan..

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It is notable for having an extremely heavy supermassive black hole at its centre, one of the largest black holes ever found. Read More » NGC 1277 in Perseus Enter a coin's NGC certification number (circled in the image) and grade to confirm its description and grade in NGC's database and, if available, view the images of the coin taken by NGC. For coins that have a grade of 1 to 70, enter the certification number, select the numeric grade in the dropdown menu and click "Go." NGC 1277 är en linsformad spiralgalax i stjärnbilden Perseus, belägen omkring 220 miljoner ljusår bort.. Den 28 november 2012 upptäckte astronomer vid Max Planck-institutet för astronomi ett supermassivt svart hål i galaxens mitt, vilket är ett av universums största hittills upptäckta, med en massa motsvarande 17 miljarder Solmassor. [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.

Black holes are again hitting the headlines. Another record super massive black hole has been unveiled. This time it is galaxy NGC 1277 at the center of which a true monster is discovered to be lurking. Dutch astronomer Remco van den Bosch and co-workers weighed the black hole at the center of this galaxy.

Otkriće: Položaj Epoha J2000.0: Zviježđe: Perzej Rektascenzija: 03 h 19 m 51.4 s: Deklinacija +41° 34′ 25″ Izgled na našem nebu: Prividna magnituda: 13,7 Prividne dimenzije (V) 1.0'x0.4' Stvarne osobine NGC 1277 is classified as a lenticular galaxy, so it is shaped like a lens, with a thicker central region that tapers away at the edges. It is only about one-tenth as large and massive as our home galaxy, the Milky Way, with a total mass (including invisible dark matter) of about 120 billion times the mass of the Sun. ngc 1277: Каталог коды: ngc 1277, pgc 12434, 2masx j03195148+4134242, mcg+07-07-064, z 540-104, z 0316.6+4123, uzc j031951.6+413425, leda 12434 һәм [bm99] 274: Ачучы яки уйлап табучы: Лоуренс Парсонс: Ачыш датасы: 4 декабрь 1875: Йолдызлык NGC 1276, yew cısmê asmêniyo.No cısım Katalogê Neweyê Pêroyi de ca gêno. 12 Kanun 1876 de terefê i ra keşıf biyo.. Bıvênên. Asmên; Galaksi; Pulsar; Nebula; Lista cısmanê NGC; Gırey teberi. Heqa NGC 1276 sitay NASA/IPAC Extragalactic Database sero bıvênê (be İngılızki); NGC 1276 sitay SIMBADi sero bıvênên (be İngılızki); Heqa NGC 1276 sitay LEDA sero bıvênê (be 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.

Qora tuynuk. 2012-yil 28-noyabrida Olmoniyaning Max Planck Astronomiya Instituti astronomlari NGC 1277 galaktikasi markazida … Nedovršeni članak NGC 1277 koji govori o astronomiji treba dopuniti. prema pravilima Wikipedije Ova stranica posljednji je put uređivana 26. siječnja 2019. u 19:57. Tekst je dostupan pod licencijom Creative Commons Imenovanje/Dijeli pod istim uvjetima; dodatni uvjeti mogu se primjenjivati. Pogledajte NGC 1277.