Sh2-297 (original) (raw)
Sh2-297 (also known as Sharpless 297) is an emission nebula in the constellation Canis Major.The region was catalogued in 1959 in the extended seconded edition of the Sharpless catalogue. This area is part of the Canis Major OB1 Association, and is a very active area of new star formation. Distance is estimated between 1.0 and 1.4 kpc. (3,300–4,600 ly.), averaging 1.2 kpc. or 3,900 ly.
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| dbo:abstract | Sh2-297 (also known as Sharpless 297) is an emission nebula in the constellation Canis Major.The region was catalogued in 1959 in the extended seconded edition of the Sharpless catalogue. This area is part of the Canis Major OB1 Association, and is a very active area of new star formation. Studies in 1988 found that the bright star illuminating the nebula was 8th magnitude HD 53623 / HIP 34178 with spectral class B1II/III. Later in 2004 it was shown that there was embedded a cold but massive Young Stellar Object or YSO within Sh2-297 near the edge of one of the dark rifts. This object has been observed in the far-infrared, but it is so deeply embedded in an interstellar cloud that it is undetectable in shorter wavelength observations such as the Two Micron All Sky Survey (2MASS), leading it to be originally named "Unidentified young stellar object 1" or UYSO-1. It was further revealed that this unseen stellar source produces a carbon monoxide (CO) bipolar outflow with a total mass of 5.4 M☉ solar masses, while the surrounding extended envelope weighs 30 M☉–40 M☉. Some 96 other YSOs have been discovered to be part of Sh-297, having a mean age of one million years and range in masses between 0.3 M☉ and 2.0 M☉. Many variable stars are also assigned with this nebula complex, including the three brightest: MW Ori, TT Ori and V559 Ori. Distance is estimated between 1.0 and 1.4 kpc. (3,300–4,600 ly.), averaging 1.2 kpc. or 3,900 ly. (en) |
| dbo:thumbnail | wiki-commons:Special:FilePath/Ced_90.jpg?width=300 |
| dbo:wikiPageID | 53465807 (xsd:integer) |
| dbo:wikiPageLength | 5272 (xsd:nonNegativeInteger) |
| dbo:wikiPageRevisionID | 1057611371 (xsd:integer) |
| dbo:wikiPageWikiLink | dbr:Carbon_monoxide dbr:Interstellar_medium dbc:Canis_Major dbc:Reflection_nebulae dbr:Light_year dbc:Sharpless_objects dbr:Palomar_Sky_Survey dbc:Star-forming_regions dbr:Bipolar_outflow dbr:IC_2177 dbr:Reflection_nebula dbr:Southern_celestial_hemisphere dbr:Sharpless_catalog dbr:Lynds'_Catalogue_of_Bright_Nebulae dbr:Star_formation dbr:Two_Micron_All_Sky_Survey dbr:Stellar_associations dbr:Young_Stellar_Object dbr:Variable_stars dbr:Kiloparsecs dbr:Canis_Major_(constellation) |
| dbp:constellation | dbr:Canis_Major_(constellation) |
| dbp:dec | -12 (xsd:integer) |
| dbp:distLy | 3300 (xsd:integer) |
| dbp:epoch | J2000.0 (en) |
| dbp:name | Sh2-297 (en) |
| dbp:names | Sh-297, LBN 1039, Ced 90 (en) |
| dbp:ra | 25513.0 |
| dbp:type | Emission (en) |
| dbp:wikiPageUsesTemplate | dbt:Canis_Major dbt:Reflist dbt:Sky dbt:Solar_mass dbt:Sh2_objects dbt:Infobox_nebula |
| dcterms:subject | dbc:Canis_Major dbc:Reflection_nebulae dbc:Sharpless_objects dbc:Star-forming_regions |
| rdfs:comment | Sh2-297 (also known as Sharpless 297) is an emission nebula in the constellation Canis Major.The region was catalogued in 1959 in the extended seconded edition of the Sharpless catalogue. This area is part of the Canis Major OB1 Association, and is a very active area of new star formation. Distance is estimated between 1.0 and 1.4 kpc. (3,300–4,600 ly.), averaging 1.2 kpc. or 3,900 ly. (en) |
| rdfs:label | Sh2-297 (en) |
| owl:sameAs | yago-res:Sh2-297 wikidata:Sh2-297 https://global.dbpedia.org/id/2qQCu |
| prov:wasDerivedFrom | wikipedia-en:Sh2-297?oldid=1057611371&ns=0 |
| foaf:depiction | wiki-commons:Special:FilePath/Ced_90.jpg |
| foaf:isPrimaryTopicOf | wikipedia-en:Sh2-297 |
| is dbo:wikiPageRedirects of | dbr:Sharpless_297 |
| is dbo:wikiPageWikiLink of | dbr:Sharpless_catalog dbr:Sharpless_297 |
| is foaf:primaryTopic of | wikipedia-en:Sh2-297 |
