NGC 1596 is a lenticular galaxy in the constellation Dorado. The galaxy lies about 55 million light years away from Earth, which means, given its apparent dimensions, that NGC 1596 is approximately 55,000 light years across. [1] It was discovered by John Herschel on December 5, 1834. [3] It is a member of the Dorado Group. [4]

NGC 1596 位于剑鱼座α星西方约1°，是一个以侧面朝向我们的小星系，分类为S0的透镜星系，视星等11.1等，蓝星等12.1等，视大小约3.7'x.9'，表面亮度12.3等，像是一个缩小版的 宽帽星系,于1834年12月5日被 约翰·弗里德里希·威廉·赫歇尔 发现。 这个星系需要14吋（35公分）以上的望远镜才能看见，一些视野较大的影像会同时呈现，星等13等，非常靠近的NGC 1602 [1]。 ^ 存档副本. [2009-08-11]. （原始内容 存档 于2008-10-15）. 维基共享资源 上的相关多媒体资源： NGC …

NGC 1596 is a Lenticular Galaxy in the Dorado constellation. NGC 1596 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its visual magnitude of 10.97, NGC 1596 is visible with the help of a telescope having an aperture of 6 inches (150mm) or more.

NGC 1596 位于剑鱼座α星西方约1°，是一个以侧面朝向我们的小星系。 分类为S0的透镜星系，视星等11.1等，蓝星等12.1等，视大小约3.7'x0.9'，表面亮度12.3等，像是一个缩小版的宽帽星系,于1834年12月5日被 约翰·弗里德里希·威廉·赫歇尔 发现。 这个星系需要用14吋（35厘米）以上的望远镜才能看见，星等13等，非常靠近 NGC 1602。 NGC 1596 位于剑鱼座α星西方约1°，是一个以侧面朝向我们的小星系。

We present Australia Telescope Compact Array (ATCA) HI imaging of the edge-on galaxy NGC 1596, which was recently found to have counter-rotating ionized gas in its center (<15"). We find a large...

NGC 1596 . NGC 1596 is a lenticular galaxy located in the constellation Dorado. Some key stats include:

Origin of the counterrotating gas in NGC 1596 We present Australia Telescope Compact Array HI imaging of the edge-ongalaxy NGC 1596, which was recently found to have counterrotatingionized gas in its centre (15 arcsec). We find a large HI envelopeassociated with a nearby companion, the dwarf irregular galaxy NGC 1602.The HI covers a region ~11. ...

We present Australia Telescope Compact Array H i imaging of the edge-on galaxy NGC 1596, which was recently found to have counterrotating ionized gas in its cen

ngc 1596 位於劍魚座α星西方約1°，是一個以側面朝向我們的小星系，分類為s0的透鏡星系，視星等11.1等，藍星等12.1等，視大小約3.7'x.9'，表面亮度12.3等，像是一個縮小版的寬帽星系,於1834年12月5日被約翰·弗里德里希·威廉·赫歇爾發現。

We have identified two new galaxies with gas counter-rotation (NGC 1596 and 3203) and have confirmed similar behaviour in another one (NGC 128), this using results from separate studies of the ionized-gas and stellar kinematics of a well-defined sample of 30 edge-on disc galaxies.