Celestial hemisphere:  Northern  ·  Constellation: Leo (Leo)  ·  Contains:  NGC 3239
Getting plate-solving status, please wait...
Arp 263, Gary Imm
Arp 263, Gary Imm

Arp 263

Getting plate-solving status, please wait...
Arp 263, Gary Imm
Arp 263, Gary Imm

Arp 263

Equipment

Loading...

Acquisition details

Loading...

Description

This beautiful and wondrous object is an irregular galaxy located 25 million light years away in the constellation of Leo. It is much smaller than our Milky Way, at a diameter of 40,000 light years. The galaxy is a bit obscured by the bright foreground Milky Way star, HD 222046.

As reflected by its Arp designation, the structure of this galaxy suggests that it has been involved in an interaction with another galaxy. The tidal star streams, bright blue star clusters, and faint Ha star forming regions also support the idea of recent galaxy interaction. Although many background galaxies are visible here, none are close enough to suggest a companion galaxy, Consequently, we are likely looking at the aftermath of a merger between two galaxies.

This galaxy is an extreme example that symmetry is not always seen in galaxies. The right galaxy tail contains many Ha regions and is bluish in color, while the left galaxy tail does not contain any Ha regions and is yellowish in color. Both tails extend below the disk. A remnant of a core appears to be towards the left side of the disk.

The most interesting part of this image to me is what appears to be a mass of large bright blue star clusters just to the left of the foreground star. This mass has been called a giant HII region by several publications, although no other detail or explanation is given. This is the first time I have seen such a disproportionately large mass of star clusters.

Comments

Revisions

  • Final
    Arp 263, Gary Imm
    Original
  • Arp 263, Gary Imm
    B

B

Description: Comparison to Original Arp Image

Uploaded: ...

Sky plot

Sky plot

Histogram

Arp 263, Gary Imm

In these collections

Arp Catalog (Complete)