WRAY 18-52
carbon star in the constellation Puppis
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WRAY 18-52
Summary
WRAY 18-52 is a carbon star[1].
Key Facts
- WRAY 18-52's instance of is recorded as carbon star[2].
- WRAY 18-52's instance of is recorded as infrared source[3].
- WRAY 18-52's instance of is recorded as near-infrared source[4].
- WRAY 18-52's instance of is recorded as variable star[5].
- WRAY 18-52's constellation is recorded as Puppis[6].
- WRAY 18-52's spectral class is recorded as C[7].
- WRAY 18-52's catalog code is recorded as CGCS 2090[8].
- WRAY 18-52's catalog code is recorded as GSC 06567-02204[9].
- WRAY 18-52's catalog code is recorded as IRAS 08081-2923[10].
- WRAY 18-52's catalog code is recorded as NSV 17764[11].
- WRAY 18-52's catalog code is recorded as [W71b] 018-07[12].
- WRAY 18-52's catalog code is recorded as 2MASS J08101001-2932028[13].
- WRAY 18-52's catalog code is recorded as UCAC2 19361902[14].
- WRAY 18-52's catalog code is recorded as Gaia DR1 5596724879298097408[15].
- WRAY 18-52's catalog code is recorded as Gaia DR2 5596724883605753728[16].
- WRAY 18-52's catalog code is recorded as V531 Pup[17].
- WRAY 18-52's catalog code is recorded as Gaia DR3 5596724883610563456[18].
- WRAY 18-52's catalog code is recorded as TIC 154837856[19].
- WRAY 18-52's catalog code is recorded as TYC 6567-2204-1[20].
- WRAY 18-52's type of variable star is recorded as semiregular variable star[21].
- WRAY 18-52's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.25'}[22].
- WRAY 18-52's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.88'}[23].
- WRAY 18-52's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.392'}[24].
- WRAY 18-52's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.785'}[25].
- WRAY 18-52's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.30'}[26].
Body
Designation and Status
Recorded instance of include carbon star[2], infrared source[3], near-infrared source[4], and variable star[5].
History and Context
Catalog codes include CGCS 2090[8], GSC 06567-02204[9], IRAS 08081-2923[10], NSV 17764[11], [W71b] 018-07[12], and 2MASS J08101001-2932028[13].