
New General Catalog Objects: NGC 2550 - 2599 - cseligman.com
2018年12月2日 · Physical Information: Based on a recessional velocity of 4740 km/sec, NGC 2599 is about 220 million light years away. Given that and its apparent size of 2.8 by 2.5 …
NGC 2599 - Spiral Galaxy in Cancer | TheSkyLive.com
NGC 2599 is a Spiral Galaxy in the Cancer constellation. NGC 2599 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain …
NGC 2599 – Wikipedia
NGC 2599 ist eine spiralförmige Radiogalaxie vom Hubble-Typ Sa im Sternbild Krebs auf der Ekliptik. Sie ist schätzungsweise 208 Millionen Lichtjahre von der Milchstraße entfernt und hat …
Galaxies with Declining Rotation Curves | Astronomy Reports
2020年4月14日 · The galaxies that exceed 1 \(\sigma \) are indicated in the figure on the right: the triangle is NGC 2599, the square is NGC 753, the cross is NGC 5055, the pentagon is NGC …
NGC天体列表 (2000-2999) - 维基百科,自由的百科全书
ngc 2336 - 这是一个大漩涡星系在北极星方向。 ngc 2346 - 这是麒麟座的一个行星状星云。 ngc 2349 - 这是麒麟座的一个疏散星团。 ngc 2359 - 托尔的头盔,这是一个星云; ngc 2360 - 这是 …
Category : NGC 2599 - Wikimedia
Media in category "NGC 2599" The following 3 files are in this category, out of 3 total.
Digitized Sky Survey (DSS) Images of NGC/IC Objects
The NGC image archive (1st pass) is now complete (23,520 images - 7840 positives, 7840 negatives, 7840 thumbnails - All annotated) - I will be updating the public database with Dr. …
용골자리 성운 - 나무위키
2025年2月6日 · 발광성운인 Gum 31또는 IC 2599에 둘러싸여 있으며 이 성운에서 약 1,200만년전 생겨났다고 추정되는 중이다. 주로 뜨겁고 매우 큰 항성 들로 이루어져 있으며 그중에는 …
New General Catalog Objects: NGC 2500 - 2549 - cseligman.com
2023年9月11日 · Physical Information: Based on a recessional velocity of 505 km/sec, NGC 2500 is about 24 million light years away, but for small distances peculiar (non-Hubble expansion) …
Gem Cluster (NGC 3293) - Constellation Guide
NGC 3324 and IC 2599 are jointly referred to as the Gabriela Mistral Nebula, after the Chilean poet. NGC 3324 lies 9,100 light-years away and has a radius of 15 light years. Both NGC …
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