NO Apodis (original) (raw)

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dbo:abstract NO Apodis is a solitary, red hued variable star located in the southern circumpolar constellation Apus. It has an average apparent magnitude of 5.86, allowing it to be faintly seen with the naked eye. The object is relatively far at a distance of 790 light years but is drifting closer with a heliocentric radial velocity −18.3 km/s. NO Apodis has a stellar classification of M3 III, indicating that it is a red giant. It is currently on the asymptotic giant branch, fusing hydrogen and helium shells around an inert carbon core. At present it has 1.63 times the mass of the Sun and an enlarged radius of 107 R☉. It shines with a bolometric luminosity 1,408 times that of the Sun from its photosphere at an effective temperature of 3,521 K. NO Apodis is classified as a semiregular variable of unknown subtype. Observations from Tabur et. al. (2009) reveal it to have two periods, both lasting 26-7 days. During this timeframe, the star flucates between 5.71 and 5.95 in the visual band. (en) ふうちょう座NO星(ふうちょうざNOせい、NO Apodis、NO Aps)は、ふうちょう座にある半規則型変光星(脈動変光星)である。 (ja) HD 156513,又名CP-80 828,SAO 258769、HR 6429,是一颗恒星,视星等为5.88,位于銀經312.32,銀緯-23.69,其B1900.0坐标为赤經17h 12m 45.1s,赤緯-80° -23.69′ 59″。 (zh)
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dbp:absmagV −1.32 (en)
dbp:appmagV 5.710000 (xsd:double)
dbp:bV +1.67 (en)
dbp:class M3 III (en)
dbp:constell dbr:Apus
dbp:epoch J2000 (en)
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dbp:luminosity 1408 (xsd:integer)
dbp:mass 1.630000 (xsd:double)
dbp:pError 0.074100 (xsd:double)
dbp:parallax 4.147900 (xsd:double)
dbp:propMoDec −43.943 (en)
dbp:propMoRa −3.662 (en)
dbp:radialV −18.3 (en)
dbp:radius 107 (xsd:integer)
dbp:temperature 3521 (xsd:integer)
dbp:type dbr:Asymptotic_giant_branch
dbp:uB +1.80 (en)
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rdfs:comment ふうちょう座NO星(ふうちょうざNOせい、NO Apodis、NO Aps)は、ふうちょう座にある半規則型変光星(脈動変光星)である。 (ja) HD 156513,又名CP-80 828,SAO 258769、HR 6429,是一颗恒星,视星等为5.88,位于銀經312.32,銀緯-23.69,其B1900.0坐标为赤經17h 12m 45.1s,赤緯-80° -23.69′ 59″。 (zh) NO Apodis is a solitary, red hued variable star located in the southern circumpolar constellation Apus. It has an average apparent magnitude of 5.86, allowing it to be faintly seen with the naked eye. The object is relatively far at a distance of 790 light years but is drifting closer with a heliocentric radial velocity −18.3 km/s. NO Apodis is classified as a semiregular variable of unknown subtype. Observations from Tabur et. al. (2009) reveal it to have two periods, both lasting 26-7 days. During this timeframe, the star flucates between 5.71 and 5.95 in the visual band. (en)
rdfs:label ふうちょう座NO星 (ja) NO Apodis (en) HD 156513 (zh)
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foaf:name NO Apodis (en)
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