Skip to content
Surf Wiki
Save to docs
general/cepheus-constellation

From Surf Wiki (app.surf) — the open knowledge base

Sh 2-155

H II region in the constellation Cepheus

Sh 2-155

Summary

H II region in the constellation Cepheus

FieldValue
nameSh 2-155
imageCaveHunterWilson.jpg
captionSh 2–155
typeEmission
epochJ2000.0
ra22h 57m 17.14s
dec+62° 28′ 33.4"
dist_ly2400
appmag_v7.7
size_v50.0'x30.0'
constellationCepheus
radius_ly35
absmag_v16
namesSh 2-155, Caldwell 9, LBN 110.11+02.44

Sh 2-155 (also designated Caldwell 9, Sharpless 155 or S155, or LBN529) is a diffuse nebula in the constellation Cepheus, within a larger nebula complex containing emission, reflection, and dark nebulosity. It is widely known as the Cave Nebula, though that name was applied earlier to Ced 201, a different nebula in Cepheus. Sh 2-155 is an ionized H II region with ongoing star formation activity, at an estimated distance of 725 parsecs (2400 light-years) from Earth.

Sh 2-155{{cite simbad |access-date=11 March 2017}} was first noted as a galactic emission nebula in 1959 in the extended second edition of the Sharpless catalogue,{{cite journal

Sh 2-155 lies at the edge of the Cepheus B cloud (part of the Cepheus molecular cloud), and is ionized by young stars from the Cep OB3 association.{{Cite journal

Other name designations

Amateur photograph of the Cave Nebula in the [[Hubble palette

The name "Cave Nebula" was coined for this object by Patrick Moore, presumably derived from photographic images showing a curved arc of emission nebulosity corresponding to a cave mouth.{{Cite book |access-date=11 March 2017}} or VdB 152,{{cite simbad |access-date=12 March 2017}}{{cite web |access-date=11 March 2017}} positioned at R.A.: 22h 13m 27s Dec.: +70° 15′ 18″ (2000). The name's application to Sh 2-155 has come into vogue through the nebula's inclusion in Moore's Caldwell catalogue{{cite book

References

References

  1. (2006). "ChandraStudy of the Cepheus B Star-forming Region: Stellar Populations and the Initial Mass Function". The Astrophysical Journal Supplement Series.
  2. (1959). "Photoelectric Photometry of the Association III Cephei.". The Astrophysical Journal.
  3. (1970). "Four-color and H-beta photometry of open clusters - VI - the association III Cep.". The Astronomical Journal.
  4. Patrick Moore (1990). ''The Amateur Astronomer'' (11th ed), W.W. Norton & Company, {{ISBN. 0-393-02864-X
  5. (August 12, 2009). "Cepheus B: Trigger-Happy Star Formation".
  6. (2009). "Protoplanetary Disk Evolution Around the Triggered Star-Forming Region Cepheus B". The Astrophysical Journal.
Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

Want to explore this topic further?

Ask Mako anything about Sh 2-155 — get instant answers, deeper analysis, and related topics.

Research with Mako

Free with your Surf account

Content sourced from Wikipedia, available under CC BY-SA 4.0.

This content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.

Report