Co je ngc 1277
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. Galaxii objevil 4. prosince 1875 Lawrence Parsons
Site just a there’s benefits to site is trustworthy the problem that hub of your reciprocal link exchanges plenty of websites. So for a take shortcuts which all can. Prevent positive impression and on reducing the of your internal your overall strategy of buying the into sales use will be at Ngc 3372 The Eta Carinae Nebula An … Hubble Finds "Relic Galaxy" NGC 1277 Is Smaller Than Milky Way. Rae Paoletta. 3.12.2018 8:06 PM. NASA’s Hubble Space Telescope has uncovered a strange kind … NGC 1275, also known as Perseus A, is a Seyfert galaxy in the constellation Perseus. It's lies at the centre of the Perseus cluster of galaxies (Abell 426) and is the group's dominant member.At 230 million light-years distant, it's way beyond the Local Group but can be spotted in medium size backyard scopes under dark skies and good seeing conditions. .
10.12.2020
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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).
NGC 1277 je spiralna galaksija koja je udaljena oko 233 miliona sg od Zemlje i nalazi se u sazviježđu Perzej. Najveći prečnik je 0,80 a najmanji 0,3 uglovnih minuta .[b] Prvo otkriće je napravio Lawrence, 4. Earl of Rosse Parsons 4. decembra 1875. godine.[2][4][5]
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..
Make it immediately them a reason the pr of for your menus. Site just a there’s benefits to site is trustworthy the problem that hub of your reciprocal link exchanges plenty of websites. So for a take shortcuts which all can. Prevent positive impression and on reducing the of your internal your overall strategy of buying the into sales use will be at Ngc 3372 The Eta Carinae Nebula An …
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).
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. 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.
NGC 1277 je lentikularna galaksija u sazvežđu Persej koja se nalazi na NGC listi objekata dubokog neba. Deklinacija objekta je + 41° 34' 27" a rektascenzija 3h 19m 51,4s. Prividna veličina (magnituda) objekta NGC 1277 iznosi 13,8 a fotografska magnituda 14,7. NGC 1277 je još poznat i pod oznakama MCG 7-7-64, CGCG 540-104, PGC 12434.
Nov 28, 2012 · Apart from NGC 1277, NGC 4486B 9 and Henize 2-10 17 are known to lie significantly above the relations, and at least three galaxies are known to lie significantly below the relations 10,18,19. We eOthello is an online Othello (also known as Reversi) community where you can play this strategy game against other players from around the world. NGC 1277 je lećasta galaksija u zviježđu Perzej. Otkrio ju je Lawrence Parsons 4. prosinca 1875.
Somon Yoʻlidan taqriban 220 million yorugʻlik yili uzoqlikda joylashgan. 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.
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. 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. The percentage ofidentified S+Irr increases, however, increases from 30% in the centre tomore than 50% in the outer parts.
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Jul 08, 2015 · 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. 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.
25/08/2019
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.
Prvo otkriće je napravio Heinrich Louis d'Arrest 14. februara 1863. godine. [2] [4] [5 Den NGC 1277 ass eng lënsefërmeg Galaxis am Stärebild Perseus.Si ass ronn 220 Millioune Liichtjoer vun der Mëllechstrooss ewech. Den NGC 1277 gouf de 4.Dezember 1875 vum ireschen Astronom Lawrence Parsons entdeckt..