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. T1 - On the Spiral Structure of NGC 5248: An Analytic Approach. AU - Yuan, Chi. AU - Yang, Chao-Chin.
Sie ist schätzungsweise 50 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 95.000 Lichtjahren. T1 - On the Spiral Structure of NGC 5248: An Analytic Approach. AU - Yuan, Chi. AU - Yang, Chao-Chin. PY - 2006. Y1 - 2006.
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.
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.
NASA called out the notable ring structure around its nucleus, indicating starburst activity. "Starburst regions are sites where stars form at a Nedovršeni članak NGC 5248 koji govori o astronomiji treba dopuniti. prema pravilima Wikipedije Ova stranica posljednji je put uređivana 22.
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. Picture Details: Optics 32-inch Schulman Telescope (RC Optical Systems) Camera SBIG STX CCD Camera Filters AstroDon Generation II Dates
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
Selected data and derived quantities for NGC 5248 †. More information in the tabs above.
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AU - Yuan, Chi. AU - Yang, Chao-Chin. PY - 2006. Y1 - 2006. N2 - An improved nonlinear asymptotic theory of spiral density waves is developed.
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ngc 5248 — спирална галаксија во соѕвездието Воловар, заведена во Новиот општ каталог на објекти на длабокото небо.. Телото било предмет и на други истражувања, па освен како ngc 5248 се споменува и како ugc 8616, mcg 2-35-15, cgcg 73-54, iras
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..
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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.