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 structure encircling the bar that is interacting with NGC 2535.

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 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 Spirals with companions on arms – large, high surface brightness companions class, these peculiar spirals are located approximately 200 million light-years away ...

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 elongated structure, visible at ultraviolet wavelengths, that contain many bright, recently formed blue star clusters in addition to enhanced star forming regions ...

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 transform spectrometer (iFTS) SITELLE attached to the Canada-France-Hawaii Telescope (CFHT), are presented.

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 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 visual magnitude of 13.93, NGC 2536 is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.

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 the Atlas of Peculiar Galaxies as an example of a spiral galaxy with a …

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 gas and five clouds with masses of ∼ 10 8 M ⨀ in the tidal arms of NGC 2535.

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 (30 km s -1) in the H I gas and five clouds with masses of ∼108 Msun in the tidal arms of NGC 2535.