
NGC 2536 - Wikipedia
NGC 2536 is a barred spiral galaxy in the constellation Cancer. It was discovered on 22 January 1877 by French astronomer Édouard Stephan. [2] NGC 2536 has a prominent inner ring …
NGC 2536 - 维基百科,自由的百科全书
ngc 2536位於巨蟹座,是正與ngc 2535進行交互作用中的一個棒旋星系。 這兩個星系被一起列在 特殊星系圖集 中,是螺旋星系與高表面亮度星系作用的一個例子 [ 2 ] 。
Arp 82 - Experienced Deep Sky Imaging - Cloudy Nights
Arp 82 consists of NGC 2535 (UGC 4264, VV 9a and others), the center spiral with the extended arm and NGC 2536 (PGC 22958, VV 9b and others), the companion below it. Part of Arp’s …
NGC 2535 - Wikipedia
NGC 2535 is exhibiting a weak inner ring structure around the nucleus that is interacting with NGC 2536. The interaction has warped the disk and spiral arms of NGC 2535, producing an …
The interacting pair of galaxies Arp 82: integral field ... - NASA/ADS
Spectral data cubes of the interacting pair of galaxies NGC 2535 and NGC 2536 (the Arp 82 system) targeting bright emission lines in the visible band, obtained with the imaging Fourier …
NGC 2536 GalaxyFacts - Universe Guide
NGC 2536 (NGC2536) is a barred spiral galaxy that has a distance from Earth of light years. It can be found in the constellation of Cancer.
NGC 2536 - Spiral Galaxy in Cancer | TheSkyLive.com
NGC 2536 is a Spiral Galaxy in the Cancer constellation. NGC 2536 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its …
NGC 2536 - Wikiwand
NGC 2536 is a barred spiral galaxy with a prominent inner ring structure encircling the bar in the constellation Cancer that is interacting with NGC 2535. The two galaxies are listed together in …
Ocular Galaxies: Ngc 2535 and Its Starburst Companion Ngc 2536 …
NGC 2535 has an ocular (eye-shaped) structure indicative of a recent, close, nonmerging encounter. Our observations reveal widespread high velocity dispersions (30 kms -1) in the HI …
Observations of the Ocular Galaxy NGC 2535 and its Starburst Companion ...
NGC 2535 has an ocular (eye-shaped) structure with two long tidal arms indicative of a recent, close, nonmerging encounter. Our observations reveal widespread high velocity dispersions …