RCW 14
Coordinates: (235.6°, -4.1°)
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RCW 14 appears to be a visible part of the [JKK96] B giant molecular cloud and is part of the GS234-02 supershell. The main ionising star is the O8 V star HD 57236.
Avedisova lists 3 additional B-class ionising stars and places RCW 14 in the star formation region SFR 235.54-4.06 along with the star cluster NGC 2367. The RCW catalog also associates RCW 14 with NGC 2367.
Kharchenko gives a distance of 2004 parsecs and an age of 10.2 million years for NGC 2367.
Avedisova lists 3 additional B-class ionising stars and places RCW 14 in the star formation region SFR 235.54-4.06 along with the star cluster NGC 2367. The RCW catalog also associates RCW 14 with NGC 2367.
Kharchenko gives a distance of 2004 parsecs and an age of 10.2 million years for NGC 2367.
The exciting star is the O8 V star HD 57236. [1]
More on the GS234-02 supershell. [2]
Bica, et.al. find a 55 solar mass star cluster in this direction ([BBD2004] Cluster 3) at a distance of 3930 +/- 350 pc. They conclude that it is a background object lying behind the nebula. The same paper adds that RCW 14 appears to be the nucleus of the larger nebula Brand 16. [3]
More on the GS234-02 supershell. [2]
Bica, et.al. find a 55 solar mass star cluster in this direction ([BBD2004] Cluster 3) at a distance of 3930 +/- 350 pc. They conclude that it is a background object lying behind the nebula. The same paper adds that RCW 14 appears to be the nucleus of the larger nebula Brand 16. [3]
Notes
1. ^ Yamaguchi, Reiko, Saito, Hiro, Mizuno, Norikazu, et al. (1999). "Molecular Clouds and Star Formation in the Southern H II Regions", Publications of the Astronomical Society of Japan, Vol. 51, 791-818. [1999PASJ...51..791Y]
2. ^ Jung, Jae Hoon, Koo, Bon-Chul, & Kang, Yong-Hee (1996). "GS234-02: A Star Forming Supershell in the Outer Galaxy", The Astronomical Journal, Vol. 112, 1625. [1996AJ....112.1625J]
3. ^ Bica, E., Bonatto, C., & Dutra, C. M. (2004). "Discovery of three optical open clusters in the Galaxy", Astronomy and Astrophysics, Vol. 422, 555-562. [2004A&A...422..555B]
Distance estimates
2500 pc [1996AJ....112.1625J]Links
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Most of the sources used to create these nebula descriptions are listed in the
notes section for each description. In some cases,
for example the Avedisova, Humphreys and Reed catalogs, the source is used extensively and is not listed in the
individual nebula descriptions. See this catalog overview
for more information on the catalogs and the general sources used
to create these descriptions and this introduction to HII regions
on the general history of this area of astronomy.
This image was created using the POSS-II/UKSTU data of the Digitized Sky Survey and SuperCOSMOS using the process described here.
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and this acknowledgement taken from the DSS site:
The Digitized Sky Surveys were produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions.
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