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However recent observations in the near infra-red have shown that in fact there may be a much longer bar with intense star formation which may … NGC 5248 (također poznat kao IRAS 13350+0908, MCG 2-35-15, PGC 48130 i UGC 8616) je prečkasta spiralna galaksija koja je udaljena oko 53 miliona sg od Zemlje i nalazi se u sazviježđu Volar.Najveći prečnik je 6,20 (95 hiljada sg) a najmanji 4,5 uglovnih minuta (69 hiljada sg). Prvo otkriće je napravio John Frederick William Herschel 15. aprila 1784. godine.

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NGC 5248 je prečkasta spiralna galaktika u zviježđu Volaru. Izvori Vanjske poveznice. engl.) SEDS: NGC 5248 (engl.) Revidirani Novi opći katalog (engl NGC 5248 (aliaj indikoj — UGC 8616, MCG 2-35-15, ZWG 73.54, IRAS13350+0908, PGC 48130) estas galaksio en konstelacio Bovisto.. Ĉi tiu objekto estis jam en la originala versio de NGC-katalogo. ngc 5248: Каталоган код: ngc 5248, iras 13353+0908, pgc 48130, ugc 8616, 2masx j13373206+0853062, iras f13350+0908, mcg+02-35-015, sdss j133732.02+085306.6, uzc j133732.0+085308, z 1335.0+0908, z 73-54, alfalfa 3-552, hipass j1337+08, leda 48130 NGC 5248 main frame - University of Washington NGC 5248 Волопас yulduz turkumidagi SBbc tipli galaktikadir. Ushbu obyekt Yangi umumiy katalog asl nashrida mavjud.

NGC 5248 (ayrıca Caldwell 45 olarak da bilinir), Başak takımyıldızı yönünde yaklaşık olarak 50 milyon ışık yılı uzaklıkta bulunan bir çubuklu sarmal galaksi.

"Starburst regions are sites where stars form at a ngc 5248 — Дохкаллин а, седарчийн гуламийн а керла юкъара каталогехь ягарйина галактикаш. NGC 5248 (Caldwell 45) is another great example.

Ngc 5248

"Starburst regions are sites where stars form at a ngc 5248 — Дохкаллин а, седарчийн гуламийн а керла юкъара каталогехь ягарйина галактикаш. NGC 5248 (Caldwell 45) is another great example. NASA called out the notable ring structure around its nucleus, indicating starburst activity. "Starburst regions are sites where stars form at a NGC 5248 је спирална галаксија у сазвежђу Волар која се налази на NGC листи објеката дубоког неба..

Ngc 5248

NGC 5248 (còn được gọi là Caldwell 45) là một thiên hà xoắn ốc trung gian nhỏ gọn cách chúng ta khoảng 59 triệu năm ánh sáng trong chòm sao Boötes. Nó là thành viên của Nhóm thiên hà NGC 5248 , bản thân nó là một trong những nhóm Virgo III được kéo dài về phía đông của Siêu đám Xử Nữ . [2] NGC 5248 је спирална галаксија у сазвежђу Волар која се налази на NGC листи објеката дубоког неба. Деклинација објекта је + 8° 53' 10" а ректасцензија 13h 37m 32,0s.
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Ngc 5248

NGC 4775, Image · Spectrum, NGC 5248, Image · Spectrum. NGC 5548, Image · Spectrum, NGC  Nearly all (>80%) of the star formation in NGC 1326 and NGC 4314 is contained in the circumnuclear rings, whereas NGC 1512 and NGC 5248 have actively star-   Jul 8, 2019 Here is an image of the galaxy NGC 5248 - a member of the Virgo Cluster of Galaxies.

Fiv… Media in category "NGC 5248" The following 3 files are in this category, out of 3 total. NGC 5248 spirálgalaxis: Megfigyelési adatok: Csillagkép: Bootes: Rektaszcenzió: 13 h 37 m 32,1 s: Deklináció +08° 53′ 06″ Vöröseltolódás: 0,003846: Távolság: 74 millió fényév fé, 13 550 000 pc: Típus (R)SB(rs)bc: Más elnevezések: Caldwell 45 ngc 5248 (المعروفة أيضا باسم كالدويل 45) هي مجرة حلزونية متوسطة تقع في كوكبة العواء تبعد حوالي 59 مليون سنة ضوئية.
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William Herschel tarafından 15 Nisan 1784 tarihinde keşfedilmiştir. Galaksi, Başak III Grupları'nın bir alt-grubu olan NGC 5248 Grubu üyesidir ve etkin bir galaksidir.

Picture Details: Optics 32-inch Schulman Telescope (RC Optical Systems) Camera SBIG STX CCD Camera Filters AstroDon Generation II Dates March 3rd and 4th NGC 5248 uploaded in EAA goodies: CPC800 f/6.3 ASI 178 MM 45 x 8 sec no filters High gain location Stuttgart Germany 2021.03.23/24 NGC 5248 (UGC 8616, PGC 48130, Caldwell 45 and others) is a spiral galaxy located approximately 44 million (https://iopscience.i56/152/2/50/pdf) light-years away in Boötes. MCG+02-35-014 (PGC 48114 and others) is the Seyfert 2 ring galaxy at the top center. On the Spiral Structure of NGC 5248: An Analytic Approach An improved nonlinear asymptotic theory of spiral density waves isdeveloped. It extends the theory developed by Yuan & Kuo to a globaltheory, not just one limited to the vicinity of the resonance. NGC 5248 is in the constellation of Bootes but is actually part of the Virgo cluster of galaxies.

Abstract. We present for the first time a two-dimensional velocity field of the central region of the grand-design spiral galaxy NGC 5248, at 0.9-arcsec spatial. NGC 5248. De Vaucouleurs Atlas Type: (R')SAB(rs)bc. Filter: B. Telescope: INT 2.5-m. North up , East left. Field Dimensions: 8.3 x 7.2 arcminutes.