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. RC3 Type: 

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.

engl.) SEDS: NGC 5248 (engl.) Revidirani Novi opći katalog (engl 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. Manbalar. Havolalar. NGC 5248 NGC 5248 ist eine aktive Balken-Spiralgalaxie mit ausgedehnten Sternentstehungsgebieten vom Hubble-Typ SBbc[2] und liegt im Sternbild Bootes an der Grenze zum Sternbild Jungfrau. Sie ist schätzungsweise 50 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 95.000 Lichtjahren.

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NGC 5247 is a face-on unbarred spiral galaxy located some 60 million light years away in the constellation Virgo.It most likely belongs to the Virgo Supercluster of galaxies; the same supercluster that hosts the Milky Way galaxy. NGC 5248 (také známá jako Caldwell 45) je spirální galaxie v souhvězdí Pastýře vzdálená přibližně 50 milionů světelných let.Objevil ji britský astronom William Herschel v roce 1784. 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 (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.

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

These spirals contain 1.2  Dec 11, 2020 Spiral galaxy NGC 5248 is listed as Caldwell 45 in the catalog. The freshly processed Hubble image shows off its stunning form. NASA, ESA, J. NGC 3627, Image · Spectrum, NGC 3941, Image · Spectrum. NGC 4775, Image · Spectrum, NGC 5248, Image · Spectrum.

Caldwell 45, or NGC 5248, is a spiral galaxy located in the constellation Boötes, and it is notable for the ring structure around its nucleus. These nuclear rings are characterized by “hot spots” of starburst activity. Starburst regions are sites where stars form at a much higher rate than usual.

Referințe [ modificare | modificare sursă ] 1999-01-01 Ο NGC 5248 ή Caldwell 45 είναι ενδιάμεσος σπειροειδής γαλαξίας ο οποίος απέχει 59 εκατομμύρια έτη φωτός από την Γη και βρίσκεται στον αστερισμό Βοώτης.Ανήκει στην Ομάδα γαλαξιών NGC 5248, που ονομάστηκε πήρε το όνομά της από αυτόν. 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. Привидна величина (магнитуда) објекта NGC 5248 износи 10,1 а фотографска 1997-11-01 NGC 5248 je prečkasta spiralna galaksija koja je udaljena oko 53 miliona sg od Zemlje i nalazi se u sazviježđu Volar.

NGC 5249 · Bootes. NGC 5248 is a compact intermediate spiral galaxy about 59 million light-years away in the constellation Boötes.
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Najveći prečnik je 6,20 a najmanji 4,5 uglovnih minuta .[b] Prvo otkriće je napravio John Frederick William Herschel 15. aprila 1784. godine.[2][4][5] Definitions of NGC_5248, synonyms, antonyms, derivatives of NGC_5248, analogical dictionary of NGC_5248 (Italian) NGC 5248 galaxia espiral bat da, Boötes konstelazioan.

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. Manbalar.
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NGC 5248 (left) is a spiral galaxy and one of the brightest galaxies in this region. NGC 5363 (centre) is a lenticular galaxy with a faint lane of dust passing through  

The Carnegie-Irvine Galaxy Survey (CGS). Data Products. Images . • summary from image atlas. • original FITS images (B, V, R, I). 13 May 2015 This close-up video sequence shows the huge elliptical galaxy NGC 5128 (also known as Centaurus A). This object is the closest such galaxy  GASDYNAMICS IN NGC 5248: FUELING A CIRCUMNUCLEAR STARBURST RING.

NGC 5248. Picture Details: Optics 32-inch Schulman Telescope (RC Optical Systems) Camera SBIG STX CCD Camera Filters AstroDon Generation II Dates March 3rd and 4th

AU - Yuan, Chi. AU - Yang, Chao-Chin. PY - 2006. Y1 - 2006. N2 - An improved nonlinear asymptotic theory of spiral density waves is developed. It extends the theory developed by Yuan & Kuo to a global theory, not just one limited to the vicinity of the resonance. NGC 5248 ist eine aktive Balken-Spiralgalaxie mit ausgedehnten Sternentstehungsgebieten vom Hubble-Typ SBbc und liegt im Sternbild Bootes an der Grenze zum Sternbild Jungfrau. Sie ist schätzungsweise 50 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 95.000 Lichtjahren.

الانزياح الأحمر: 0.00384. السرعه الشعاعيه: 1151. المطلع المستقيم: 204.3836208. الميل: 8.8850611. NGC 5248 est une galaxie spirale de type Sc dans la constellation du Bouvier, située à environ 15 Mpc (∼48,9 millions d'a.l.) de la Terre.. Déjà bien visible dans un 115 mm, elle mérite que l'on s'attarde dessus, en photo ou en numérique.