Astronomy:NGC 2174
Emission nebula | |
---|---|
H II region | |
File:NGC-2174.tif Monkey Head Nebula in Narrowband Sulfur-Hydrogen Alpha- Oxygen with a 1000mm telescope | |
Observation data: J2000 epoch | |
Right ascension | 06h 09.7m[1] |
Declination | +20° 30′[1] |
Distance | 6,400[citation needed] ly (2,000 pc) |
Constellation | Orion |
NGC 2174 (also known as Monkey Head Nebula) is an H II[1] emission nebula located in the constellation Orion and is associated with the open star cluster NGC 2175.[1] It is thought to be located about 6,400 light-years away from Earth. The nebula may have formed through hierarchical collapse.[2]
There is some equivocation in the use of the identifiers NGC 2174 and NGC 2175. These may apply to the entire nebula, to its brightest knot, or to the star cluster it includes. Burnham's Celestial Handbook lists the entire nebula as 2174/2175 and does not mention the star cluster.[3] The NGC Project (working from the original descriptive notes) assigns NGC 2174 to the prominent knot at J2000 06h 09m 23.7s, +20° 39′ 34″ and NGC 2175 to the entire nebula, and by extension to the star cluster.[4] Simbad uses NGC 2174 for the nebula and NGC 2175 for the star cluster.[1] [5]
Glowing gas and dark dust do not survive well in the Monkey Head Nebula. Young stars near the center of the nebula generate stellar winds and high energy radiation that causes the nebula's material to shift into complex shapes.[6] The nebula is primarily composed of hydrogen which glows at infrared wavelengths due to the radiation.[7]
Hubble 24th Anniversary Images (2014)
Gallery
Infrared image of NGC 2174 as viewed by the Spitzer Space Telescope
References
- ↑ 1.0 1.1 1.2 1.3 1.4 "NGC 2174". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+2174.
- ↑ Cotera, A.; Hester, J.; Healy, K.; Snider, K.; Simpson, J.; Whitney, B. (August 2006). "Using Spitzer IRAC observations to Compare Modes of Star Formation in G305.35+0.7 and NGC 2174/5". Triggered Star Formation in a Turbulent ISM, International Astronomical Union Symposium. Prague, Czech Republic (published 2006). S237, #98. Bibcode: 2006IAUS..237E..98C.[|permanent dead link|dead link}}]
- ↑ Robert Burnham, Jr, Burnham's Celestial Handbook, Dover, 1978, p. 1280.
- ↑ "Public Database". Results for NGC 2174 and NGC 2175. http://www.ngcicproject.org/pubdb.htm.
- ↑ "SIMBAD Astronomical Database". Results for NGC 2175. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=ngc+2175&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id.
- ↑ "Monkey See, Monkey Do". Astronomy 42: 10. Aug 4, 2014.
- ↑ "Pillars in the Monkey Head Nebula". Mar 17, 2014. https://hubblesite.org/contents/media/images/3887-Image?Collection=Hubble%20Heritage&page=3.
- ↑ "Hubble Celebrates 24th Anniversary with Infrared Image of Nearby Star Factory". 2014-03-17. https://www.nasa.gov/press/2014/march/hubble-celebrates-24th-anniversary-with-infrared-image-of-nearby-star-factory/.
External links
- NASA Astronomy Picture of the Day: NGC 2174: Emission Nebula in Orion (8 December 2006)
- NASA Astronomy Picture of the Day: NGC 2174: Stars Versus Mountains (9 February 2011)
- NASA Astronomy Picture of the Day: At the Edge of NGC 2174 (3 April 2014)
- Monkey Head Nebula at Constellation Guide
- Monkey Head Nebula in the Staracle NGC catalog
Original source: https://en.wikipedia.org/wiki/NGC 2174.
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