Celestial hemisphere:  Northern  ·  Constellation: Vulpecula (Vul)  ·  Contains:  HD186930  ·  HD186998  ·  HD338833  ·  HD338835  ·  HD338915  ·  HD338917  ·  HD338918  ·  HD338924  ·  HD338925  ·  HD338926  ·  LBN 137  ·  LBN 138  ·  LBN 139  ·  Sh2-88
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Sh2 88, 88B1 and 88B2, Jerry Yesavage
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Sh2 88, 88B1 and 88B2

Getting plate-solving status, please wait...
Sh2 88, 88B1 and 88B2, Jerry Yesavage
Powered byPixInsight

Sh2 88, 88B1 and 88B2

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Description

From GalaxyMap:

This nebula associated with the Vul OB1 association consists of three regions - star formation began in a diffuse large nebula Sh 2-88A, then spread to the compact HII region Sh 2-88B1, ionised by an O8.5-9.5 V star, and then finally spread to the ultracompact Sh 2-88B2, ionised by a star dimmer than B0.5 V.

Avedisova lists three ionising stars: the O7 V star HD 338916, the O8.5 Ib supergiant HD 338926, and the B0.5 V star LS II +25 09.

From Wikipedia:

Sharpless 2-88 or Sh 2-88 is a region including the [url=mw-redirect=https://en.wikipedia.org/wiki/Diffuse_nebula]diffuse nebula[/url] Sh 2-88A and the two compact knots Sh 2-88B1 and Sh 2-88B2, all of which are associated with Vulpecula OB1.Sh 2-88A is an HII-type diffuse nebula excited by the type O8 star BD+25°3952.=reference[4] Both neutral and ionized gases in Sh 2-88 are between 150 and 410 solar masses and the dust mass is about 2 to 9 solar masses. The structure been interacting with a HI interstellar bubble shaped by the stellar winds of BD+25°3952 and the blue O8.5II(f) star BD +25°3866. Overall, its actual structure is located 2.4 kiloparsecs away, at 23 × 15 parsecs in radius. It has a dynamical age of 1.5 million years, and a mass of 1,300 solar masses. It has an rms electron density of 9 cm−3. All separate star forming regions are 1 arcminute in diameter.=reference[5]

Sharpless 2-88 is the first part of this nebula to have created a star-forming region. It had star formation first start in this large diffuse nebula, which then spread to the other star-forming regions in the nebula.

It spread to the compact Sharpless 2-88B1, then to the ultracompact Sharpless 2-88B2.

Sharpless 2-88B1 is a HII region ionized by an O8.5-9.5 V star, and is compact. It is also associated with a nearby star cluster that contains several massive stars.Sharpless 2-88B2 is a HII region ionized by a star that is dimmer than B0.5 V, and is ultracompact.=reference[6]

I think the two bright areas in the lower left are the two star formation areas (B1 and B2) noted above.  Think they are labeled 88A and 88B in the photo.

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Previous version shows a lot more stars... I toned them down in this version:

Sh2 88 H-alpha RGB

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