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词条 Sharpless 2-88
释义

  1. Nearby objects

  2. References

{{Multiple issues|{{context|date=June 2016}}{{lead rewrite|date=June 2016}}
}}{{Infobox nebula
| name = Sharpless 2-88
| type = diffuse
| subtype = Reflection/Emission[1]
| epoch = Epoch J2000
| ra =19h 45m 59s[2]
| dec = 25° 20' 00"[3]
| dist_ly = 6,523
| dist_pc = 2400 [4]
| constellation = Vulpecula
| radius = 345
| absmag_v = --
| names = LBN 139, The Face of God Nebula
|size=47 light years across}}Sharpless 2-88, also known as Sh 2-88, is a region of diffuse nebulae northwest of the nebula knots Sh 2-88A, Sh 2-88B1, and Sh 2-88B2, which are all associated with Vulpecula OB1. This nebula is a HII type diffuse nebula excited by the type O8 star BD +26°3952.[5] Both neutral and ionized gases in Sh 2-88 are between 150 and 410 Msolar and the dust mass is about 2 to 9 Msolar. The nebula is ionized by an O8.5 to 9.5V star. The structure been interacting with a HI interstellar bubble shaped by the stellar winds of BD +26°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, a dynamical age of 1.5 million years, and a mass of 1,300 Msolar. It has an rms electron density of 9 cm–3. All separate star forming regions are 1 minute in diameter.[6]

Nearby objects

(All of the nebulae mentioned are in the Vulpecula OB1 association.)

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.[7]

HD 338916 is an emission line star that ionizes a close nebula in the Vulpecula OB1 association. It has an apparent magnitude (V) of 10.17 and a spectral type of O8 D.

HD 338926 is another emission line star that ionizes a close nebula in the Vulpecula OB1 association. It has an apparent magnitude (V) of 9.55 and a spectral type of O8e C.

References

1. ^http://mschuster.zenfolio.com/p126650821/h683135D9#h683135d9
2. ^http://dso-browser.com/dso/info/Sh/2-88/bright-nebula
3. ^http://dso-browser.com/dso/info/Sh/2-88/bright-nebula
4. ^http://galaxymap.org/cat/view/sharpless/88
5. ^http://mschuster.zenfolio.com/p126650821/h683135D9#h683135d9
6. ^http://billsnyderastrophotography.com/?page_id=4051
7. ^{{Cite web|url=http://galaxymap.org/cat/view/sharpless/88|title=Sh 2-88|website=galaxymap.org|access-date=2017-04-03}}
{{nebula-stub}}

3 : Vulpecula|Nebulae|Star-forming regions

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