ugc 9618（或称为vv 340或arp 302）包含一对富含气体处于撞击早期的旋涡星系，其中vv 340a是左边侧向的星系，vv 340b 是右边正向的星系 观测资料（ J2000 曆元 ）

Arp 302, also known as VV 340 or UGC 9618 consists of a pair of very gas-rich spiral galaxies in their early stages of interaction. An enormous amount of infrared light is radiated by the gas from massive stars that are forming at a rate similar to the most vigorous giant star-forming regions in our own Milky Way .

UGC 9618又被稱為VV 340或Arp 302，位於牧夫座，由兩個富含氣體，處於撞擊早期的旋渦星系組成。 兩個星系的氣體受大質量 恆星 作用輻射出大量的 紅外線 。

2008年4月24日 · UGC 9618 is 450 million light-years away from Earth, and is the 302nd galaxy in Arp's Atlas of Peculiar Galaxies. This image is part of a large collection of 59 images of merging galaxies taken by the Hubble Space Telescope and released on the occasion of its 18th anniversary on 24th April 2008.

UGC 9618 is 450 million light-years away from Earth, and is the 302nd galaxy in Arp's Atlas of Peculiar Galaxies. This image is part of a large collection of 59 images of merging galaxies taken by the Hubble Space Telescope and released on the …

2008年4月24日 · An enormous amount of infrared light is radiated by the gas from massive stars that are forming at a rate similar to the most vigorous giant star-forming regions in our own Milky Way. UGC 9618 is 450 million light-years away from Earth, and is the 302nd galaxy in Arp's Atlas of Peculiar Galaxies.

UGC 9618又被称为VV 340或Arp 302，位于 牧夫座，由两个富含气体，处于撞击早期的 旋涡星系 组成。 两个星系的气体受大质量 恒星 作用辐射出大量的 红外线。 这些大质量恒星的形成率与 银河系 最大、最活跃的恒星形成区相似。 UGC 9618距离地球4.5亿光年远，在Arp（特殊星系图集）中排名第302。 位于北边正向我们的星系又被成为MCG +04-35-019、UGC 9618N或UGC 9618B。 UGC 9618又被称为VV 340或Arp 302，位于牧夫座，由两个富含气体，处于撞击早 …

UGC 9618 is 450 million light-years away from Earth, and is the 302nd galaxy in Arp's Atlas of Peculiar Galaxies. This image is part of a large collection of 59 images of merging galaxies taken by the Hubble Space Telescope and released on the …

UGC 9618距离地球4.5亿光年远，在Arp（特殊星系图集）中排名第302。 UGC 9618又被称为VV 340或Arp 302，位于牧夫座，由两个富含气体，处于撞击早期的旋涡星系组成。

UGC 9618, also known as VV 340 or Arp 302 consists of a pair of very gas-rich spiral galaxies in their early stages of interaction: VV 340A is seen edge-on to the left, and VV 340B face-on to the right.