Sh 2-50
Also called
RCW 164Coordinates: (16.93°, -1.07°)
[ Catalog | Explorer | SIMBAD ]
Sh 2-50 appears in the direction of the Sct OB3 association and the star cluster Dolidze 28, which has the Wolf-Rayet star WR 115 as its central star.
Avedisova places Sh 2-50 in the star formation region SFR 16.90-1.06 along with the star cluster Dolidze 28.
She says that the nebula is ionised by the Wolf-Rayet star MR 115. [1] However, MR 115 is located in a completely different location and this seems to be a typo for the Wolf-Rayet star WR 115, which SIMBAD notes as the central star of Dolidze 28.
Interestingly, Sh 2-50 is prominent at hydrogen-alpha and radio frequencies but is not visible in MSX infrared images.
The radio image may in fact be showing the supernova remnant SNR G16.8-1.1. G16.8-01.1 and the microquasar LS 5039 lie behind Sh 2-50 at a distance of 2900 pc. [2]
A 2011 paper looked at the relationship between SNR G16.8-1.1 and the hydrogen-alpha emission in this direction and found no clear association, providing further evidence that the supernova remnant is a distinct object. [3]
She says that the nebula is ionised by the Wolf-Rayet star MR 115. [1] However, MR 115 is located in a completely different location and this seems to be a typo for the Wolf-Rayet star WR 115, which SIMBAD notes as the central star of Dolidze 28.
Interestingly, Sh 2-50 is prominent at hydrogen-alpha and radio frequencies but is not visible in MSX infrared images.
The radio image may in fact be showing the supernova remnant SNR G16.8-1.1. G16.8-01.1 and the microquasar LS 5039 lie behind Sh 2-50 at a distance of 2900 pc. [2]
A 2011 paper looked at the relationship between SNR G16.8-1.1 and the hydrogen-alpha emission in this direction and found no clear association, providing further evidence that the supernova remnant is a distinct object. [3]
Notes
1. ^ Avedisova, V. S. & Kondratenko, G. I. (1984). "Exciting stars and the distances of the diffuse nebulae", Nauchnye Informatsii, Vol. 56, 59. [1984NInfo..56...59A]
2. ^ Ribó, M., Paredes, J. M., Romero, G. E., et al. (2002). "
3. ^ Stupar, M. & Parker, Q. A. (2011). "Catalogue of known Galactic SNRs uncovered in Hα light", Monthly Notices of the Royal Astronomical Society, Vol. 414, 2282-2296. [2011MNRAS.414.2282S]
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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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Use of these images is courtesy of the UK Schmidt Telescope (copyright in which is owned by the Particle Physics and Astronomy Research Council of the UK and the Anglo-Australian Telescope Board) and the Southern Sky Survey as created by the SuperCOSMOS measuring machine and are reproduced here with permission from the Royal Observatory Edinburgh.
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.
The compressed files of the "Palomar Observatory - Space Telescope Science Institute Digital Sky Survey" of the northern sky, based on scans of the Second Palomar Sky Survey are copyright ? 1993-1995 by the California Institute of Technology and are distributed herein by agreement. The compressed files of the "Palomar Observatory - Space Telescope Science Institute Digital Sky Survey" of the northern sky, based on scans of the Second Palomar Sky Survey are copyright ? 1993-1995 by the California Institute of Technology and are distributed herein by agreement.