Sh 2-219
Coordinates: (159.36°, 2.6°)
[ Catalog | Explorer | SIMBAD ]
Avedisova concludes that Sh 2-219 is ionised by the stars LS V +47 24 (O9.5 V) and LS V +47 22 (B0 V).
The nebula is very young - perhaps only about 100 thousand years old. There is also an embedded star cluster to the southwest and a nearby 2000 solar mass molecular cloud
Russeil places Sh 2-219 in the same star formation complex as Sh 2-217 and BFS 44.
The nebula is very young - perhaps only about 100 thousand years old. There is also an embedded star cluster to the southwest and a nearby 2000 solar mass molecular cloud
Russeil places Sh 2-219 in the same star formation complex as Sh 2-217 and BFS 44.
The nebula is very young - perhaps only about 100 thousand years old. There is also an embedded star cluster to the southwest and a nearby 2000 solar mass molecular cloud. [1]
This is ionised by a B0 V star, Sh 2-219 no. 194, in an embedded star cluster. [2]
Russeil places Sh 2-219 in the same star formation complex as Sh 2-217 and BFS 44. [3]
This is ionised by a B0 V star, Sh 2-219 no. 194, in an embedded star cluster. [2]
Russeil places Sh 2-219 in the same star formation complex as Sh 2-217 and BFS 44. [3]
Notes
1. ^ Deharveng, L., Lefloch, B., Massi, F., et al. (2006). "Triggered massive-star formation on the borders of Galactic H II regions. III. Star formation at the periphery of Sh2-219", Astronomy and Astrophysics, Vol. 458, 191-201. [2006A&A...458..191D]
2. ^ Deharveng, L., Zavagno, A., Salas, L., et al. (2003). "Sequential star formation at the periphery of the H II regions Sh 217 and Sh 219", Astronomy and Astrophysics, Vol. 399, 1135-1145. [2003A&A...399.1135D]
3. ^ Russeil, D., Adami, C., & Georgelin, Y. M. (2007). "Revised distances of Northern HII regions", Astronomy and Astrophysics, Vol. 470, 161-171. [2007A&A...470..161R]
Distance estimates
4200 pc [1982ApJS...49..183B]4200 pc +/- 600 [1984NInfo..56...59A]
3990 pc +/- 390 [2007A&A...470..161R]
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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.
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