NGC 6694: Difference between revisions

From Citizendium
Jump to navigation Jump to search
imported>Thorsten Alteholz
(Data removed as it is not clear whether they may be used with CZ licence.)
mNo edit summary
 
(4 intermediate revisions by 3 users not shown)
Line 1: Line 1:
{{subpages}}
{{subpages}}
'''NGC 6694'''. also  known as '''M 26''', is a [[Open cluster]] located in constellation [[Scutum]].
'''NGC 6694'''. also  known as '''M 26''', is an [[open cluster]] located in the constellation [[Scutum]].
{{Infobox NGCobject
{{Infobox NGCobject
| number= NGC 6694
| number= NGC 6694
Line 6: Line 6:
| type = [[Open cluster]]
| type = [[Open cluster]]
| epoch = 2000.0
| epoch = 2000.0
| ra =  
| ra = 18 h 45.2 m
| de =  
| de = −9° 24′
| app_size =  
| app_size =  
| app_mag =
| app_mag = 8.0
| distance_ly =
| distance_ly =
| const = Scutum
| const = Scutum
Line 19: Line 19:
}}
}}
=== Appearance ===
=== Appearance ===
This is an open cluster; its brightest stars are of magnitude 11.9.  This cluster has a well-defined zone of low star density near the nucleus.  This is probably due to intervening dark interstellar matter rather than being a gap in the cluster.


=== Location ===
=== Location ===
Line 25: Line 26:


=== References ===
=== References ===
{{reflist}}
{{reflist}}[[Category:Suggestion Bot Tag]]

Latest revision as of 07:00, 23 September 2024

This article is a stub and thus not approved.
Main Article
Discussion
Related Articles  [?]
Bibliography  [?]
External Links  [?]
Citable Version  [?]
 
This editable Main Article is under development and subject to a disclaimer.

NGC 6694. also known as M 26, is an open cluster located in the constellation Scutum.

NGC 6694
Observation data: 2000.0 epoch
Constellation Scutum
Right ascension 18 h 45.2 m
Declination −9° 24′
Type Open cluster
Apparent magnitude 8.0
Other designations M 26

Appearance

This is an open cluster; its brightest stars are of magnitude 11.9. This cluster has a well-defined zone of low star density near the nucleus. This is probably due to intervening dark interstellar matter rather than being a gap in the cluster.

Location

Scientific research

References