RCW 134
Also called
Sh 2-15, Gum 69, W25Coordinates: (358.34°, -1.85°)
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This HII region is ionised by the O8 V star HD 161853 and is part of the Sh 2-15 to Sh 2-20 complex of HII regions located in the Sgr OB5 association in the Sagittarius arm. It is the location of the radio source W25.
Avedisova places it in star formation region SFR 358.44-1.88 with 2 masers and the star cluster VDBH 249. (However, SIMBAD identifies VDBH 249 as a globular cluster.)
Sh 2-15 is also called W25, Gum 69, or RCW 134. [1]
Also called RCW 134, this HII region is at a distance of 1600 pc and ionised by the O8 V star HD 161853. [2]
Although distance estimates place Sh 2-15 at approximately the same distance as Sh 2-16 to Sh 2-20, it is brighter and located further below the galactic plane than the other nebulae.
Sh 2-15 is also called W25, Gum 69, or RCW 134. [1]
Also called RCW 134, this HII region is at a distance of 1600 pc and ionised by the O8 V star HD 161853. [2]
Although distance estimates place Sh 2-15 at approximately the same distance as Sh 2-16 to Sh 2-20, it is brighter and located further below the galactic plane than the other nebulae.
Notes
1. ^ Gray, A. D. (1994). "The Most Galactic Center Survey - Part Two - New Results on Published Supernova Remnants and G:2.4+1.4", Monthly Notices of the Royal Astronomical Society, Vol. 270, 835. [1994MNRAS.270..835G]
2. ^ 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]
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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.
The Second Palomar Observatory Sky Survey (POSS-II) was made by the California Institute of Technology with funds from the National Science Foundation, the National Geographic Society, the Sloan Foundation, the Samuel Oschin Foundation, and the Eastman Kodak Corporation.
The UK Schmidt Telescope was operated by the Royal Observatory Edinburgh, with funding from the UK Science and Engineering Research Council (later the UK Particle Physics and Astronomy Research Council), until 1988 June, and thereafter by the Anglo-Australian Observatory. The blue plates of the southern Sky Atlas and its Equatorial Extension (together known as the SERC-J), as well as the Equatorial Red (ER), and the Second Epoch [red] Survey (SES) were all taken with the UK Schmidt.
The "Second Epoch Survey" of the southern sky was made by the Anglo-Australian Observatory (AAO) with the UK Schmidt Telescope. Plates from this survey have been digitized and compressed by the ST ScI. The digitized images are copyright ? 1993-5 by the Anglo-Australian Observatory Board, and are distributed herein by agreement.
The "Equatorial Red Atlas" of the southern sky was made with the UK Schmidt Telescope. Plates from this survey have been digitized and compressed by the ST ScI. The digitized images are copyright ? 1992-5, jointly by the UK SERC/PPARC (Particle Physics and Astronomy Research Council, formerly Science and Engineering Research Council) and the Anglo-Australian Telescope Board, and are distributed herein by agreement.
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