Sh 2-115
Coordinates: (84.83°, 3.91°)
[ Catalog | Explorer | SIMBAD ]
This HII region lies in the same direction as the radio source W71 and is ionised by the O6 Ib supergiant LS III +46 12 which is part of the star cluster Berkeley 90. The cloud surrounding Berkeley 90 (part of which is visible as Sh 2-115) contains 4400 solar masses of gas and dust and is about 30 pc long.
Infrared observations reveal a large, complex structure with multiple bubbles as can be seen in this MSX image. The nebula is also prominent at radio frequencies.
Infrared observations reveal a large, complex structure with multiple bubbles as can be seen in this MSX image. The nebula is also prominent at radio frequencies.
LS III +46 12 is part of the open cluster Berkeley 90. BD+46 2972 is unlikely to ionise the nebula because it is located much further away (3400 pc). The cloud surrounding Berkeley 90 (part of which is visible as Sh 2-115) contains 4400 solar masses of gas and dust and is about 30 pc long. The cluster and nebula are located at a distance of 2300 pc.[1]
This is in the same direction as the radio source W71.[SIMBAD]
This nebula has three exciting stars - DM46 2972 (O9.5 V), DM 46 2978 (B0III) and LS III 46 12 (O6). It is located at an estimated distance of 2300 pc.[2]
Avedisova gives an O6 Ib class for LS III +46 12. [3]
This is in the same direction as the radio source W71.[SIMBAD]
This nebula has three exciting stars - DM46 2972 (O9.5 V), DM 46 2978 (B0III) and LS III 46 12 (O6). It is located at an estimated distance of 2300 pc.[2]
Avedisova gives an O6 Ib class for LS III +46 12. [3]
Notes
1. ^ Harten, R. & Felli, M. (1980). "The evolved H II Region S 115", Astronomy and Astrophysics, Vol. 89, 140-144. [1980A&A....89..140H]
2. ^ Felli, M. & Harten, R. H. (1981). "A high-resolution search for small-scale structure in Sharpless H II regions at 4.995 GHz. II - General properties of the entire sample. III - Description of selected sources", Astronomy and Astrophysics, Vol. 100, 28-58. [1981A&A...100...28F]
3. ^ Avedisova, V. S. & Kondratenko, G. I. (1984). "Exciting stars and the distances of the diffuse nebulae", Nauchnye Informatsii, Vol. 56, 59. [1984NInfo..56...59A]
Distance estimates
2300 pc [1981A&A...100...28F]2950 pc +/- 520 [1984NInfo..56...59A]
3000 pc +/- 600 [1984ApJ...279..125F]
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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.
According to my correspondence with the Royal Observatory Edinburgh and the Space Telescope Science Institute, I am allowed to use the POSS-II/UKSTU data to create and display images for non-commercial purposes so long as I include this fine print for the SuperCOSMOS data:
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.