Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  

































Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 References  





2 External links  














NGC 3608






العربية
Azərbaycanca
Беларуская
Bosanski
Deutsch
Esperanto
Euskara
Français
Hrvatski
Қазақша
Македонски
مصرى
Nederlands
Нохчийн
Oʻzbekcha / ўзбекча
Polski
Português
Русский
Slovenčina
Српски / srpski
Srpskohrvatski / српскохрватски
Татарча / tatarça
Türkçe
Українська
Zazaki
 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 




In other projects  



Wikimedia Commons
 
















Appearance
   

 





Coordinates: Sky map11h16m58.967s, +18° 08 54.71
 

From Wikipedia, the free encyclopedia
 


NGC 3608
SDSS image of NGC 3608
Observation data (J2000 epoch)
ConstellationLeo
Right ascension11h16m 58.967s[1]
Declination+18° 08′ 54.71″[1]
Redshift0.003959[2]
Heliocentric radial velocity1185 ± 46 km/s[2]
Distance73 Mly (22.3 Mpc)[3]
GrouporclusterLeo II group
Apparent magnitude (V)10.76[3]
Apparent magnitude (B)11.7[2]
Absolute magnitude (V)−20.98[3]
Characteristics
TypeE1-2[3]
Other designations
UGC 6299, MCG +03-29-022, PGC 34433[2]

NGC 3608 is an elliptical galaxy located in the constellation Leo. It was discovered by William Herschel on March 14, 1784.[4]

NGC 3608 is part of the Leo II Group of galaxies, including NGC 3605 and NGC 3607. It is approximately 13.0 billion years old. There is diffuse X-ray emission coming from this galaxy and NGC 3607, which suggests that the two may be merging.[3]

NGC 3608 has a significant population of globular clusters. The population distribution is bimodal, with "red" and "blue" populations; the blue globular clusters form a majority. The blue globular clusters have a more extended distribution throughout the galaxy. Overall, the globular clusters are aligned along an axis that is not the same as the rest of the stars, which may be further evidence of galaxy interaction with NGC 3607.[3]

A large structure of neutral hydrogen gas known as an H I region, about 130,000 light-years (40 kpc) across, exists some twelve arcminutes (corresponding to about 230,000 light-years, or 70 kpc) away from NGC 3608. It may be associated with the galaxy.[5]

References[edit]

  1. ^ a b Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
  • ^ a b c d "NGC 3608". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-08-26.
  • ^ a b c d e f Kartha, Sreeja S.; Forbes, Duncan A.; Alabi, Adebusola B.; Brodie, Jean P.; Romanowsky, Aaron J.; Strader, Jay; Spitler, Lee R.; Jennings, Zachary G.; Roediger, Joel C. (2016). "The SLUGGS survey: Exploring the globular cluster systems of the Leo II group and their global relationships". Monthly Notices of the Royal Astronomical Society. 458 (1): 105–126. arXiv:1602.01838. Bibcode:2016MNRAS.458..105K. doi:10.1093/mnras/stw185.
  • ^ Seligman, Courtney. "New General Catalogue objects: NGC 3600 - 3649". cseligman.com. Retrieved 2021-08-26.
  • ^ Oosterloo, Tom; Morganti, Raffaella; Crocker, Alison; Jütte, Eva; Cappellari, Michele; De Zeeuw, Tim; Krajnović, Davor; McDermid, Richard; Kuntschner, Harald; Sarzi, Marc; Weijmans, Anne-Marie (2010). "Early-type galaxies in different environments: An H i view". Monthly Notices of the Royal Astronomical Society. 409 (2): 500–514. arXiv:1007.2059. Bibcode:2010MNRAS.409..500O. doi:10.1111/j.1365-2966.2010.17351.x. S2CID 2119031.
  • External links[edit]



  • t
  • e

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=NGC_3608&oldid=1196850733"

    Categories: 
    Leo (constellation)
    NGC objects
    Elliptical galaxies
    Principal Galaxies Catalogue objects
    Elliptical galaxy stubs
    Hidden categories: 
    Articles with short description
    Short description matches Wikidata
    Commons category link from Wikidata
    All stub articles
     



    This page was last edited on 18 January 2024, at 18:06 (UTC).

    Text is available under the Creative Commons Attribution-ShareAlike License 4.0; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profit organization.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki