dbo:abstract |
W Canis Majoris (W CMa) is a carbon star in the constellation Canis Major. A cool star, it has a surface temperature of around 2,900 K and a radius 234 times that of the Sun, with a bolometric absolute magnitude of −4.13 and distance estimated at 443 or 445 parsecs (1,444–1,450 light-years) based on bolometric magnitude or radius. The Gaia Data Release 2 parallax of 1.8049±0.1454 milliarcseconds implies a distance of about 555 parsecs. W CMa is classified as a slow irregular variable star. Detailed analyses have found only very weak and probably spurious periods of approximately a month. It is a carbon star, an asymptotic giant branch star where carbon and s-process elements have been dredged up to the surface during thermal pulses of the helium-burning shell. (en) W Canis Majoris är en halvregelbunden variabel av SR-typ i stjärnbilden Stora hunden. Stjärnan varierar mellan magnitud +6,27 och 7,09 (fotografisk magnitud) med en period av 160 dygn. (sv) W Большого Пса (лат. W Canis Majoris), HD 54361 — одиночная переменная звезда в созвездии Большого Пса на расстоянии приблизительно 1807 световых лет (около 554 парсеков) от Солнца. Видимая звёздная величина звезды — от +6,98m до +6,39m. (ru) |
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wiki-commons:Special:FilePath/WCMaLightCurve.png?width=300 |
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dbp:appmagV |
6.350000 (xsd:double) |
dbp:bV |
+2.55 (en) |
dbp:class |
C6,3 (en) |
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dbr:Canis_Major |
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dbr:J2000.0 |
dbp:equinox |
J2000.0 (en) |
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0 (xsd:integer) |
dbp:luminosity |
3560 (xsd:integer) |
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0.145400 (xsd:double) |
dbp:parallax |
1.804900 (xsd:double) |
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2.280000 (xsd:double) |
dbp:propMoRa |
−6.518 (en) |
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23 (xsd:integer) |
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234 (xsd:integer) |
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dbr:Slow_irregular_variable |
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dct:subject |
dbc:Asymptotic-giant-branch_stars dbc:Canis_Major dbc:Durchmusterung_objects dbc:Henry_Draper_Catalogue_objects dbc:Hipparcos_objects dbc:Objects_with_variable_star_designations dbc:Slow_irregular_variables dbc:Carbon_stars |
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rdfs:comment |
W Canis Majoris är en halvregelbunden variabel av SR-typ i stjärnbilden Stora hunden. Stjärnan varierar mellan magnitud +6,27 och 7,09 (fotografisk magnitud) med en period av 160 dygn. (sv) W Большого Пса (лат. W Canis Majoris), HD 54361 — одиночная переменная звезда в созвездии Большого Пса на расстоянии приблизительно 1807 световых лет (около 554 парсеков) от Солнца. Видимая звёздная величина звезды — от +6,98m до +6,39m. (ru) W Canis Majoris (W CMa) is a carbon star in the constellation Canis Major. A cool star, it has a surface temperature of around 2,900 K and a radius 234 times that of the Sun, with a bolometric absolute magnitude of −4.13 and distance estimated at 443 or 445 parsecs (1,444–1,450 light-years) based on bolometric magnitude or radius. The Gaia Data Release 2 parallax of 1.8049±0.1454 milliarcseconds implies a distance of about 555 parsecs. (en) |
rdfs:label |
W Canis Majoris (en) W Большого Пса (ru) W Canis Majoris (sv) |
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wiki-commons:Special:FilePath/WCMaLightCurve.png |
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wikipedia-en:W_Canis_Majoris |
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W Canis Majoris (en) |
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