Bobinas P4G
  • Login
  • Public

    • Public
    • Groups
    • Popular
    • People

A color image of three widely separated galaxies. The galaxy at the upper left is an edge-on spiral, seen as a thin rectangular shape with a light brown dust lane going through the middle. A translucent, curved plume, about two times the length of the galaxy trails off to the left. The galaxy at lower left is a face-on barred spiral galaxy, with a bright central bar and two spiral arms, which form an S-shape. The galaxy at lower right is a nearly face-on spiral, with a bright nucleus and curving dust lanes. The image is very dense with foreground stars. A scale bar marking 50 kpc takes up about 1/6 of the width of the image.

Download link

https://cdn.masto.host/astrodonsocial/media_attachments/files/111/914/920/821/736/508/original/dc832ecaab1effc7.png

Notices where this attachment appears

  1. Kelly Lepo (kellylepo@astrodon.social)'s status on Sunday, 11-Feb-2024 22:36:59 UTC Kelly Lepo Kelly Lepo
    in reply to

    NGC 3628, the galaxy in the upper left, likely had an encounter with NGC 3627 (M66) a few hundred million years ago, creating a dramatic tail-like plume.

    Gravitational interactions between the three galaxies in the Leo triplet may also be responsible for NGC 3627’s distorted shape and prominent spiral arms.

    📷 Fig. 1 from:
    https://ui.adsabs.harvard.edu/abs/2022A%26A...658A..25W/abstract
    3/

    In conversation Sunday, 11-Feb-2024 22:36:59 UTC from astrodon.social permalink
  • Help
  • About
  • FAQ
  • Privacy
  • Source
  • Version
  • Contact

Bobinas P4G is a social network. It runs on GNU social, version 2.0.1-beta0, available under the GNU Affero General Public License.

Creative Commons Attribution 3.0 All Bobinas P4G content and data are available under the Creative Commons Attribution 3.0 license.