宇宙之舞——M51蜗..宇宙之舞——M51蜗状星系与NGC5195 Whirlpool Galaxy在这幅图像中,遥远的星系M51(中偏右蓝色星系)和它的伴星系(N51左侧黄色星系)在引力的作用下恍如宇宙中两个舞伴,正绕着一
The Whirlpool Galaxy (Messier 51) and NGC 5195Education
A magnitude 13.0 lenticular galaxy (type S0?) in Centaurus NGC 5194 (= PGC 47404 = M51), The Whirlpool Galaxy (also, withNGC 5195=Arp 85) Charles Messier Johann Bode Charles Messier John Herschel Canes Venatici Historical Identification: Per Dreyer, NGC 5194 (= GC 3572 = JH 1622, M51, ...
density contrast (arm/interarm) to range from 1.8 to 3, comparable to results from N-body simulations of the galaxy's tidal encounter with NGC 5195... HW Rix,MJ Rieke - 《Astrophysical Journal》 被引量: 379发表: 1993年 HST Observations of Dust and Star-Forming Regions in the Ocular Ga...
this paper offers reconstructions of the orbits and outer shapes of four specific interacting pairs: Arp 295, M51 + NGC 5195, NGC 4676, and NGC 4038/... A Toomre,J Toomre - 《Astrophysical Journal》 被引量: 2469发表: 1972年 The 2MASS Large Galaxy Atlas We further showcase NGC 253 and...
A 14th-magnitude lenticular galaxy (type S0??) in Andromeda (RA 01 52 50.6, Dec +36 13 24) Historical Identification: Per Dreyer, NGC 709 (= GC 5195, Dreyer (using Lord Rosse's 72-inch telescope), 1860 RA 01 44 35, NPD 54 28.6) is "very faint, pretty small, between 2 stars...
宇宙之舞——M51蜗..宇宙之舞——M51蜗状星系与NGC5195 Whirlpool Galaxy在这幅图像中,遥远的星系M51(中偏右蓝色星系)和它的伴星系(N51左侧黄色星系)在引力的作用下恍如宇宙中两个舞伴,正绕着一
PIXEL ANALYSIS OF THE INTERACTING S0 GALAXY NGC 5195 (M51B)doi:10.1088/0004-637X/754/2/80Lee, Joon HyeopKim, Sang ChulRee, Chang HeeKim, MinjinJeong, HyunjinLee, Jong ChulKyeong, JaemannThe Astrophysical Journal
ASTRONOMY AND ASTROPHYSICS NGC 5195 - a look into the hot dusty ISM of an interacting SB0 galaxy with ISOCAM ?Boulade, OSauvage, MAltieri, BBlommaert, JGallais, PGuest, SMetcalfe, LOtt, K Okumura STran, D
Was the Whirlpool (M51) a Spiral Galaxy before the Encounter with the Companion NGC 5195?Using the B-I color index in the radial photometry of M51, applied to defined azimuthal sectors, we reveals asymmetries in the shape of the density pattern of the galactic arms. The anomalous shape is ...