2024年1月23日 · Spiral galaxies UGC 05028 and UGC 05029, collectively known as Arp 300, are captured in a new photo from the Hubble Space Telescope, showcasing rapid star formation triggered by the interaction...

2024年1月24日 · UGC 05028显示出一个明亮的结节，可能是另一次正在进行的星系合并的结果，科学家预测一旦完成，另一个星系的残余物将被UGC 05028完全吸收，从而促进新的恒星形成。

2024年1月23日 · UGC 05029 has a pronounced spiral structure and multiple hot, blue giant stars visible on the side facing UGC 05028. This enhanced star formation is likely due to the interaction between the...

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2024年1月23日 · UGC 05029具有明显的螺旋结构，在面向UGC 05028的一侧可以看到多个炽热的蓝色巨星。 这种增强的恒星形成很可能是由于两个星系之间的相互作用。

Arp 300 consists of two interacting galaxies, UGC 05028 (the smaller face-on spiral galaxy) and UGC 05029 (the larger face-on spiral). Likely due to its gravitational dance with its larger partner, UGC 05028 has an asymmetric, irregular structure, which is not as visible from ground-based telescopes but is quite distinct in this new image from ...

2024年1月24日 · UGC 05029 has a pronounced spiral structure and multiple hot, blue giant stars visible on the side facing UGC 05028. This enhanced star formation is likely due to the interaction between the two galaxies.

Galaxies spirales UGC 05028 et UGC 05029, également connues sous le nom d'Arp 300, capturées par le télescope spatial Hubble. Cette image montre la formation rapide d'étoiles déclenchée par l'interaction entre ces galaxies.

Spiral galaxies UGC 05028 and UGC 05029, also known as Arp 300, captured by the Hubble Space Telescope. This image shows the rapid star formation triggered by the interaction between these galaxies.

UGC 05029 has a pronounced spiral structure and multiple hot, blue giant stars visible on the side facing UGC 05028. This enhanced star formation is likely due to the interaction between the two galaxies.