Trying to image SH2-209 (Joe Matthews)

Trying to image SH2-209

Revision title: NGC1528 and SH2-209

I have been trying to process this data for the past few days and just to bring out the colors I wanted has been very tough, but I think this version is the best for now. I broke the image down to two cropped images of my Original image. I like the way they turned out.
.,.
SH2-209:
Sh 2-209Coordinates: (151.6°, -0.2°)[ [url=http://galaxymap.org/cat/list/sharpless/201]Catalog | Explorer | SIMBAD ]This large and dusty star formation region in the outer galaxy contains the infrared star cluster [url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=[BDS2003]+65&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id][BDS2003] 65[/url].

Avedisova places Sh 2-209 in star formation region 151.60-0.24 with 14 components including a water maser, the young stellar object IRAS 04064+5052 (CPM 12) and numerous infrared and radio sources.

Chini and Wink find three ionising stars: [CW84] S209-1(B1III), [CW84] S209-2 (O9 III), and [CW84] S209-3 (B1).

This MSX infrared image shows that Sh 2-209 appears to be the brightest spot on the edge of a bubble, which is confirmed by this recent WISE infrared image(Sh 2-209 is at the left).Very large (a diameter of about 50 pc) for an HII region in the outer galaxy. [[url=http://galaxymap.org/cat/view/sharpless/209#note_1]1]

Contains the infrared star cluster [BDS2003] 65. [[url=http://galaxymap.org/cat/view/sharpless/209#note_2]2]

Chini and Wink paper on ionising stars. [[url=http://galaxymap.org/cat/view/sharpless/209#note_3]3]Notes 1. ^ Omar, A., Chengalur, J. N., & Anish Roshi, D. (2002). "Multi-frequency GMRT observations of the H II regions S 201, S 206, and S 209. Galactic temperature gradient", Astronomy and Astrophysics, Vol. 395, 227-232. [[url=http://adsabs.harvard.edu/abs/2002A%26A...395..227O]2002A&A...395..227O] 2. ^ Bica, E., Dutra, C. M., Soares, J., et al. (2003). "New infrared star clusters in the Northern and Equatorial Milky Way with 2MASS", Astronomy and Astrophysics, Vol. 404, 223-232. [[url=http://adsabs.harvard.edu/abs/2003A%26A...404..223B]2003A&A...404..223B] 3. ^ Chini, R. & Wink, J. E. (1984). "The galactic rotation outside the solar circle", Astronomy and Astrophysics, Vol. 139, L5-L8. [[url=http://adsabs.harvard.edu/abs/1984A%26A...139L...5C]1984A&A...139L...5C] Distance estimates7816 pc [[url=http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003A&A...397..213P]2003A&A...397..213P]
4900 pc [[url=http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003A&A...404..223B]2003A&A...404..223B]
10000 pc [[url=http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=%201989BAICz..40...42A] 1989BAICz..40...42A]
4860 pc +/- 700 [[url=http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1973A&A....25..337G]1973A&A....25..337G]
5000 pc [[url=http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1975A&A....41..121W]1975A&A....41..121W]

@Information from http://galaxymap.org/cat/view/sharpless/209

NGC1528:

NGC 1528 is an open cluster in the constellation Perseus. It was discovered by William Herschel in 1790. It is located in the north-eastern part of the constellation, just under 3 degrees north of μ Persei. Less than 1.5° to the southeast is the open cluster NGC 1545 (m = 6.2). The NGC 1528 is clearly visible with 10x50 binoculars. 165 stars are recognised as members of NGC 1528, the brightest of which has apparent magnitude 8.7.[4]

References:

Cantat-Gaudin, T.; Anders, F. (January 2020). "Clusters and mirages: cataloguing stellar aggregates in the Milky Way". Astronomy & Astrophysics. 633: 22. arXiv:1911.07075. Bibcode:2020A&A...633A..99C. doi:10.1051/0004-6361/201936691. S2CID 208138247. A99.
Peña, J. H.; et al. (October 2019). "Study of the Open Cluster NGC 1528 Through uvby - β Photoelectric Photometry". Revista Mexicana de Astronomía y Astrofísica. 55: 203–209. Bibcode:2019RMxAA..55..203P. doi:10.22201/ia.01851101p.2019.55.02.08.
"NGC 1528". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-12-15.
Stephen James O'Meara (2007). Deep-Sky Companions: Hidden Treasures. Cambridge University Press. pp. 131–132. ISBN 9781139463737.

@information from Wikipedia (https://en.wikipedia.org/wiki/NGC_1528)

NGC1491:

NGC 1491, also known as LBN 794 or SH2-206, is an emission type bright nebula located about 9,800 light years away from Earth in the constellation of Perseus.[1] The nebula gets its deep red coloration due to many massive stars (such as BD+50 866) embedded within NGC 1491 producing large amounts of ultraviolet radiation and ionizing the hydrogen gas that makes up the nebula.[2][3]

"NGC 1491". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 21 February 2017.
[email protected]. "Emission Nebula NGC 1491". www.noirlab.edu. Retrieved 2023-11-26.
"NGC 1491". Stargazers Lounge. 2021-03-08. Retrieved 2023-11-26.

Information from Wikipedia (https://en.wikipedia.org/wiki/NGC_1491)

Original
Final
B
C
D
E

B

Title: NGC1528 and SH2-209

Description: A little closer

Uploaded: ...

C

Title: NGC1491 a zoom

Description: A little closer view

Uploaded: ...

D

Title: A crop of Sharpless 2-209

Uploaded: ...

E

Title: A different look of NGC1491

Uploaded: ...

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Status	Advanced success
Started	...
Astrometry.net job	9226393
PixInsight job	3UAO09LZXSM9MI7Z9NGR1J61GR1OT6A1
PixInsight queue size	n/a
PixInsight stage	TASK_LOG

RA (center)	04h13m42s.47
RA (top/left)	04h16m59s.10
RA (top/right)	04h09m32s.33
RA (bottom/right)	04h10m28s.71
RA (bottom/left)	04h17m47s.72

Dec (center)	+51°08′01″.4
Dec (top/left)	+51°36′38″.7
Dec (top/right)	+51°23′44″.5
Dec (bottom/right)	+50°38′57″.1
Dec (bottom/left)	+50°51′51″.6

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