Svoboda | Graniru | BBC Russia | Golosameriki | Facebook

To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

How to transfigure the Wikipedia

Would you like Wikipedia to always look as professional and up-to-date? We have created a browser extension. It will enhance any encyclopedic page you visit with the magic of the WIKI 2 technology.

Try it — you can delete it anytime.

Install in 5 seconds
4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
Great Wikipedia has got greater.
.
Leo
Newton
Brights
Milds

NGC 5775

From Wikipedia, the free encyclopedia

NGC 5775
Hubble Space Telescope image of NGC 5775, taken using the Advanced Camera for Surveys
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension14h 53m 57.653s[1]
Declination+03° 32′ 40.10″[1]
Redshift0.005607[2]
Heliocentric radial velocity1681[2]
Distance66.33 ± 13.31 Mly (20.338 ± 4.081 Mpc)[2]
Group or clusterVirgo Cluster
Apparent magnitude (V)11.34
Apparent magnitude (B)13.0
Characteristics
TypeSbc[3]
Apparent size (V)3.967' × 0.793'[1]
Other designations
UGC 9579, MCG+01-38-014, PGC 53247[3]

NGC 5775 is a spiral galaxy, a member of the Virgo Cluster, that lies at a distance of about 70 million light-years. Although the spiral is tilted away from us, with only a thin sliver in view, such a perspective can be advantageous for astronomers. For instance, astronomers have previously used the high inclination of this spiral to study the properties of the halo of hot gas[4] that is visible when the galaxy is observed at X-ray wavelengths. It is a member of the NGC 5775 Group of galaxies, itself one of the Virgo III Groups strung out to the east of the Virgo Supercluster of galaxies.[5]

One supernova has been observed in NGC 5775: SN 1996ae (type IIn, mag. 16.5).[6]

YouTube Encyclopedic

  • 1/3
    Views:
    533 109
    2 000
    2 395
  • Light Speed – fast, but slow
  • Galaktischer Dynamo
  • Astrophysical Plasma (Lecture - 07) by Professor G Srinivasan

Transcription

Interaction with NGC 5774

NGC 5775 is interacting with the nearby galaxy NGC 5774 in the form of two connecting H I bridges through which the gas is travelling from NGC 5774 to NGC 5775.[7] Faint optical emission as well as radio continuum emission are also present along the bridges.[8] It is possible that star formation is occurring between the galaxies.[7]

This system may be in the early stages of a merger.[8]

Gallery

References

  1. ^ a b c 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.
  2. ^ a b c "NED results for object NGC 5775". National Aeronautics and Space Administration / Infrared Processing and Analysis Center. Retrieved 4 February 2017.
  3. ^ a b "NGC 5775". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 4 February 2017.
  4. ^ Li, Jiang-Tao; Li, Zhiyuan; Wang, Q. Daniel; Irwin, Judith A.; Rossa, Joern (October 2008). "Chandra Observation of the Edge-on Spiral NGC 5775: Probing the Hot Galactic Disk/Halo Connection". Monthly Notices of the Royal Astronomical Society. 390 (1): 59–70. arXiv:0807.3587. Bibcode:2008MNRAS.390...59L. doi:10.1111/j.1365-2966.2008.13749.x. S2CID 15029716.
  5. ^ "The Virgo III Groups". Atlas of the Universe. Retrieved 2010-11-27.
  6. ^ Transient Name Server entry for SN 1996ae. Retrieved 30 March 2023.
  7. ^ a b Irwin, Judith; Caron, Bryan (2003). "The NGC 5775/4 Interacting System". In Shlosman, Isaac (ed.). Mass-Transfer Induced Activity in Galaxies. Cambridge University Press. p. 362. ISBN 978-0-521-54330-9.
  8. ^ a b Irwin, Judith A. (1994). "Arcs and bridges in the interacting galaxies NGC 5775/NGC 5774". The Astrophysical Journal. 429 (2): 618–633. Bibcode:1994ApJ...429..618I. doi:10.1086/174349.

External links


Stub icon

This spiral galaxy article is a stub. You can help Wikipedia by expanding it.

This page was last edited on 25 August 2023, at 05:56
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.
Contact WIKI 2
Introduction
Terms of Service
Privacy Policy