
NGC 4245 - Wikipedia
NGC 4245 is a barred lenticular galaxy with a ring [3] located in the constellation Coma Berenices. It was discovered on March 13, 1785, by the astronomer William Herschel. [5] It is a member of the Coma I Group. [6]
NGC 4245 - 維基百科,自由的百科全書 - zh.wikipedia.org
NGC 4245是一個位於后髮座的透鏡狀星系 [3] ,1785年3月13日由威廉·赫歇爾發現 [5] ,屬於 后髮座I星系群 ( 英語 : Coma I Group ) [6] 。
NGC 4245 - Lenticular Galaxy in Coma Berenices - TheSkyLive
NGC 4245 is a Lenticular Galaxy in the Coma Berenices constellation. NGC 4245 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 12.4, NGC 4245 is visible with the help of a telescope having an aperture of 8 inches (200mm) or more.
NGC 4245: one or two bars, and where does the gas inflow stop?
We have studied stellar and gaseous kinematics as well as stellar population properties in the center of the early-type barred galaxy NGC 4245 by means of integral-field spectroscopy. We have found a chemically distinct compact core, more metal-rich by a factor of 2.5 than the bulge, and a ring of young stars with the radius of 300 pc.
NGC 4245: one or two bars, and where does the gas inflow stop?.
We have studied stellar and gaseous kinematics as well as stellar population properties in the center of the early-type barred galaxy NGC 4245 by means of integral-field spectroscopy. We have found a chemically distinct compact core, more metal-rich by a factor of 2.5 than the bulge, and a ring of young stars with the radius of 300 pc.
Results of the fitting of the SAURON spectra for NGC 4245, from the left to the right – SSP-equivalent stellar ages, SSP-equivalent stellar metallicity, and stellar velocity dispersion. bar – a member of a rich, spiral-dominated group Coma I Cloud (Gregory & Thompson 1977). NGC 4245 is located in the dense part of the group, some 100kpc ...
NGC 4245 - Wikiwand
NGC 4245 is a barred lenticular galaxy with a ring located in the constellation Coma Berenices. It was discovered on March 13, 1785, by the astronomer William H...
NGC 4278, 4245, 4274, 4283, 4286, 4310(銀河・かみのけ座)
2022年3月16日 · ngc 4245はこの周辺の銀河団の中によく見られる棒構造が発達した典型的な棒渦状レンズ銀河です。 NGC 4310は変則的な渦状銀河で、核が偏心していて星団雲が連なる内部リングが見えます。
Herschel 219 NGC 4245
NGC 4245 seems to have something of an identity crisis. It has been variously classified as an irregular and as an Sb spiral. However looking at the above image, there is a very clear bar in the central regions, showing that it is a barred spiral, probably SBb.
NGC 4245 - phys.ttu.edu
NGC 4245, located in Coma Berenices, seems to have something of an identity crisis. It has been variously classified as an irregular and as an Sb spiral. However looking at the above image, there is a very clear bar in the central regions, showing that it is a barred spiral, probably SBb.