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.

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.
.
Leo
Newton
Brights
Milds

From Wikipedia, the free encyclopedia

NGC 4361
Emission nebula
Planetary nebula
NGC 4361 imaged with a 24-inch telescope
Observation data: J2000 epoch
Right ascension12h 24m 30.8s[1]
Declination−18° 47′ 5.6″[1]
Distance3,377.2±153.6[1] ly
Apparent magnitude (V)10.9[2]
Apparent dimensions (V)1.3' x 1.3'[2]
ConstellationCorvus[3]
DesignationsNGC 4361, PN G294.1+43.6
See also: Lists of nebulae

NGC 4361 (also known as the Lawn Sprinkler Nebula[4] or Garden Sprinkler Nebula) is a planetary nebula in the constellation of Corvus.[3][1][2] It is included in the Astronomical League's Herschel 400 Observing Program.

YouTube Encyclopedic

  • 1/5
    Views:
    1 527
    762
    5 875
    4 131
    6 652
  • First 2 Months Results With a Dobsonian Telescope
  • The Herschel 400 (Part 2) | Electronically-Assisted Astronomy (EAA) via a 11-Inch RASA Telescope
  • Apparent Magnitude versus Absolute Magnitude
  • Live Deep Sky Tour June 9th
  • Alpha Centauri Star versus Beta Centauri Star

Transcription

Central star

NGC 4361's central star is an extremely hot [WC] Wolf-Rayet type star. Its temperature is 126,000 K.[5] It is nearly 18,000 times brighter than the Sun, but is only 6.1% its size. This star left the asymptotic giant branch between 5776 and 8018 years ago.[5]

Gallery

References

  1. ^ a b c d "NGC 4361 -- Planetary Nebula". Simbad Astronomical Database. Universite de Strasbourg. Retrieved 6 May 2019.
  2. ^ a b c "Planetary Nebula NGC 4361". Telescopius. Retrieved 6 May 2019.
  3. ^ a b Stefan Rumistrzewicz (1 November 2010). A Visual Astronomer's Photographic Guide to the Deep Sky: A Pocket Field Guide. Springer Science & Business Media. pp. 158–. ISBN 978-1-4419-7242-2.
  4. ^ Stoyan, Ronald; Schurig, Stephan (2014). interstellarum Deep Sky Atlas. Erlangen: Cambridge University Press; Oculum-Verlag GmbH. ISBN 978-1-107-50338-0. OCLC 920437579.
  5. ^ a b González-Santamaría, I.; Manteiga, M.; Manchado, A.; Ulla, A.; Dafonte, C. (2019-10-01). "Properties of central stars of planetary nebulae with distances in Gaia DR2". Astronomy & Astrophysics. 630: A150. arXiv:1909.04601. Bibcode:2019A&A...630A.150G. doi:10.1051/0004-6361/201936162. ISSN 0004-6361.

External links


This page was last edited on 10 June 2024, at 18:17
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.