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 6309
Emission nebula
Planetary nebula
NGC 6309 as seen through the Hubble Space Telescope
Observation data: J2000 epoch
Right ascension17h 14m 04.3s[1]
Declination−12° 54′ 38″[1]
Apparent magnitude (V)11.5[2]
Apparent dimensions (V)0.32[2]
ConstellationOphiuchus
DesignationsPK 9+14.1, HD 155752, Box Nebula[3]
See also: Lists of nebulae

NGC 6309, also known as the Box Nebula, is a planetary nebula located in the constellation Ophiuchus. It was discovered by the German astronomer Wilhelm Tempel in 1876.[4] It has a luminosity of about 1800 times that of the Sun.[1][2][5] The distance to this nebula is not well known, but it is assumed to be about 6,500 light-years or 2,000 parsecs.[6]

NGC 6309 is a quadrupolar nebula, with two pairs of lobes. Surrounding the pair is a spherical shell. The spherical shell formed before the four lobes.[6] The square-like shape of the nebula gives it the nickname "Box Nebula".

The central star of the planetary nebula is an O-type star with a spectral type of O(He).[7]

See also

References

  1. ^ a b c "Object No. 1 - NGC 6309". NASA/IPAC extragalactic database. NASA/IPAC. Retrieved 4 October 2015.
  2. ^ a b c "Revised NGC Data for NGC 6309". Seds. Retrieved 4 October 2015.
  3. ^ "NGC 6309". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-03-21.
  4. ^ Seligman, Courtney. "NGC 6309, the Box Nebula". cseligman.com. Retrieved 4 October 2015.
  5. ^ "NGC 6309". Illinois.edu. Retrieved 4 October 2015.
  6. ^ a b Rubio, G.; Vázquez, R.; Ramos-Larios, G.; Guerrero, M. A.; Olguín, L.; Guillén, P. F.; Mata, H. (2015). "NGC 6309, a planetary nebula that shifted from round to multipolar". Monthly Notices of the Royal Astronomical Society. 446 (2): 1931–1938. arXiv:1410.7060. Bibcode:2015MNRAS.446.1931R. doi:10.1093/mnras/stu2201.
  7. ^ González-Santamaría, I.; Manteiga, M.; Manchado, A.; Ulla, A.; Dafonte, C.; López Varela, P. (2021). "Planetary nebulae in Gaia EDR3: Central star identification, properties, and binarity". Astronomy & Astrophysics. 656: A51. arXiv:2109.12114. Bibcode:2021A&A...656A..51G. doi:10.1051/0004-6361/202141916. S2CID 237940344.

External links


This page was last edited on 26 January 2024, at 01:39
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.