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Sh 2-155

From Wikipedia, the free encyclopedia
(Redirected fromS 155)
H II region in the constellation Cepheus
Sh 2-155
Emission nebula
Sh 2–155
Observation data: J2000.0epoch
Right ascension22h 57m 17.14s
Declination+62° 28′ 33.4"
Distance2400 ly
Apparent magnitude (V)7.7
Apparent dimensions (V)50.0'x30.0'
ConstellationCepheus
Physical characteristics
Radius35 ly
Absolute magnitude (V)16
DesignationsSh 2-155,Caldwell 9,LBN 110.11+02.44
See also:Lists of nebulae

Sh 2-155 (also designatedCaldwell 9,Sharpless 155 orS155, orLBN529) is adiffuse nebula in the constellationCepheus, within a larger nebula complex containing emission, reflection, and dark nebulosity. It is widely known as theCave Nebula, though that name was applied earlier to Ced 201, a different nebula in Cepheus. Sh 2-155 is an ionizedH II region with ongoingstar formation activity,[1] at an estimated distance of 725 parsecs (2400 light-years) from Earth.[2][3]

Sh 2-155[4] was first noted as a galactic emission nebula in 1959 in the extended second edition of theSharpless catalogue,[5] being a part of the much larger Cep OB3Association.[5] Although Sh 2-155 is relatively faint for amateur observation, some of its structure may be seen visually through a moderately sized telescope under dark skies.[6][7]

Sh 2-155 lies at the edge of the Cepheus B cloud (part of the Cepheusmolecular cloud), and isionized by young stars from the Cep OB3 association.[8] It has been suggested that radiation from the hotO-type star HD 217086 is compressing the region, triggering the formation of a new generation of stars.[9] A study of the region'syoung stellar objects by theChandra X-ray Observatory andSpitzer Space Telescope shows a progression of stellar ages in front of the cloud, supporting the hypothesis oftriggered star-formation.[10][11]

Other name designations

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Amateur photograph of the Cave Nebula in theHubble palette

The name "Cave Nebula" was coined for this object byPatrick Moore, presumably derived from photographic images showing a curved arc of emission nebulosity corresponding to a cave mouth.[12] The name was also used earlier to refer to another brighter but unrelated reflection nebula in Cepheus known as Ced 201[13] or VdB 152,[14][15] positioned atR.A.: 22h 13m 27sDec.: +70° 15′ 18″ (2000). The name's application to Sh 2-155 has come into vogue through the nebula's inclusion in Moore'sCaldwell catalogue[16] as object Caldwell 9. (SIMBAD lists the name for Ced 201, but not for Sh 2-155.)[4][13]

References

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  1. ^Getman, Konstantin V.; Feigelson, Eric D.; Townsley, Leisa; Broos, Patrick; Garmire, Gordon; Tsujimoto, Masahiro (2006). "ChandraStudy of the Cepheus B Star-forming Region: Stellar Populations and the Initial Mass Function".The Astrophysical Journal Supplement Series.163 (2):306–334.arXiv:astro-ph/0601405.Bibcode:2006ApJS..163..306G.doi:10.1086/501453.ISSN 0067-0049.S2CID 16305023.
  2. ^Blaauw, A.; Hiltner, W. A.; Johnson, H. L. (1959). "Photoelectric Photometry of the Association III Cephei".The Astrophysical Journal.130: 69.Bibcode:1959ApJ...130...69B.doi:10.1086/146697.ISSN 0004-637X.
  3. ^Crawford, D. L.; Barnes, J. V. (1970). "Four-color and H-beta photometry of open clusters - VI - the association III Cep".The Astronomical Journal.75: 952.Bibcode:1970AJ.....75..952C.doi:10.1086/111045.ISSN 0004-6256.
  4. ^ab"Sh2-155".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved11 March 2017.
  5. ^abSharpless, S. (1959). "A Catalogue of H II Regions".Astrophysical Journal Supplement.4: 257.Bibcode:1959ApJS....4..257S.doi:10.1086/190049.
  6. ^Patrick Moore (1990).The Amateur Astronomer (11th ed), W.W. Norton & Company,ISBN 0-393-02864-X
  7. ^Trusock, T. (11 March 2017)."The Caldwell Objects – Deep Sky Companions"(PDF).
  8. ^Panagia, N.; Thum, C. (1981). "A study of the S 155A – CEP B cloud and its relation to Cepheus OB3 association".Astronomy and Astrophysics.92 (2):295–299.Bibcode:1981A&A....98..295P.
  9. ^Minchin, Nigel R.; Ward-Thompson, Derek; White, Glenn J. (1992). "Carbon monoxide and far-infrared observations of the S 155-Cepheus B region".Astronomy and Astrophysics.265 (2):733–742.Bibcode:1992A&A...265..733M.
  10. ^"Cepheus B: Trigger-Happy Star Formation".chandra.harvard.edu. August 12, 2009. RetrievedMarch 12, 2017.
  11. ^Getman, Konstantin V.; Feigelson, Eric D.; Luhman, Kevin L.; Sicilia-Aguilar, Aurora; Wang, Junfeng; Garmire, Gordon P. (2009). "Protoplanetary Disk Evolution Around the Triggered Star-Forming Region Cepheus B".The Astrophysical Journal.699 (2):1454–1472.arXiv:0904.4907.Bibcode:2009ApJ...699.1454G.doi:10.1088/0004-637X/699/2/1454.ISSN 0004-637X.S2CID 18149231.
  12. ^Mobberley, M. (9 March 2017).The Caldwell Objects and How to Observe Them. Springer.ISBN 9781441903266.
  13. ^ab"Ced 201".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved11 March 2017.
  14. ^"VdB 152".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved12 March 2017.
  15. ^"APOD: 2012 October 31 – VdB 152: A Ghost in Cepheus".apod.nasa.gov. Retrieved11 March 2017.
  16. ^O'Meara, Stephen James (2002).The Caldwell Objects.Cambridge University Press.ISBN 978-0-521-82796-6.

External links

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