Celestial hemisphere:  Southern  ·  Constellation: Capricornus (Cap)  ·  Contains:  41 Cap  ·  M 30  ·  NGC 7099  ·  PGC 134281  ·  PGC 134286  ·  PGC 134287  ·  PGC 189260  ·  PGC 189288  ·  PGC 189338  ·  PGC 197859  ·  PGC 197875  ·  PGC 197888  ·  PGC 2817293  ·  PGC 3083187  ·  PGC 67099  ·  PGC 799056  ·  PGC 799249  ·  PGC 802418  ·  PGC 802456  ·  PGC 802636  ·  PGC 802975  ·  PGC 803334  ·  PGC 804236  ·  PGC 804601  ·  PGC 805583  ·  PGC 807472  ·  PGC 808276  ·  PGC 808369  ·  PGC 808417  ·  PGC 808711  ·  And 2 more.
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Lonely M 30, Claudio Tenreiro
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Lonely M 30

Getting plate-solving status, please wait...
Lonely M 30, Claudio Tenreiro
Powered byPixInsight

Lonely M 30

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Description

An image of the lonely globular cluster M30, well, there are a few faint galaxies around, but as an structure, it is alone. Also it is quite interesting the different colour of the stars in the cluster, a much larger image would have been ideal. I found some interesting reading that motivate to get the image, even within the obvious limitations, but it is great fun anyway.

According to the information on the web, it is one of the few globular clusters that has a retrograde orbit, which maybe tells something about its capture. Also it has a very dense core, actually one the more dense regions, and it is considered to have a collapsed centre.
It was studied by Chandra X ray sources due to this condition of core collapse.
If anyone has interest in reading a bit about that, it is in "CHANDRA X-RAY SOURCES IN THE COLLAPSED-CORE GLOBULAR CLUSTER M30 (NGC 7099), The Astrophysical Journal, 657:286Y301, 2007 March 1".
In that publication it is stated that "M30 (NGC 7099) is one of 21 Galactic globular clusters that show strong evidence of having undergone core collapse...", and gives an idea (for non experts) of the magnitude and impact of the phenomena.

Two nicer images with larger equipment are:
https://www.astrobin.com/135243/B/
https://www.astrobin.com/269168/

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  • Lonely M 30, Claudio Tenreiro
    Original
  • Final
    Lonely M 30, Claudio Tenreiro
    B

B

Description: A completely different stretching, after colour by photometric calibration, background subtraction in linear mode, the stretching to 15% and then to 22%.

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Lonely M 30, Claudio Tenreiro

In these collections

Globular Clusters