W Vulpeculae
variable star in the constellation Vulpecula
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W Vulpeculae
Summary
W Vulpeculae is a long-period variable star[1].
Key Facts
- W Vulpeculae's instance of is recorded as long-period variable star[2].
- W Vulpeculae's instance of is recorded as emission-line star[3].
- W Vulpeculae's constellation is recorded as Vulpecula[4].
- W Vulpeculae's spectral class is recorded as M5IIIe[5].
- W Vulpeculae's catalog code is recorded as GCRV 12522[6].
- W Vulpeculae's catalog code is recorded as GSC 02162-01244[7].
- W Vulpeculae's catalog code is recorded as HD 191652[8].
- W Vulpeculae's catalog code is recorded as HIC 99362[9].
- W Vulpeculae's catalog code is recorded as HIP 99362[10].
- W Vulpeculae's catalog code is recorded as IRAS 20079+2608[11].
- W Vulpeculae's catalog code is recorded as IRC +30415[12].
- W Vulpeculae's catalog code is recorded as 2MASS J20100428+2617072[13].
- W Vulpeculae's catalog code is recorded as NGC 6882 13[14].
- W Vulpeculae's catalog code is recorded as PPM 110550[15].
- W Vulpeculae's catalog code is recorded as RAFGL 2517[16].
- W Vulpeculae's catalog code is recorded as UBV M 37463[17].
- W Vulpeculae's catalog code is recorded as AG+26 2231[18].
- W Vulpeculae's catalog code is recorded as BD+25 4126[19].
- W Vulpeculae's catalog code is recorded as TYC 2162-1244-1[20].
- W Vulpeculae's catalog code is recorded as WEB 17735[21].
- W Vulpeculae's catalog code is recorded as Gaia DR2 1836358145537044992[22].
- W Vulpeculae's catalog code is recorded as W Vul[23].
- W Vulpeculae's type of variable star is recorded as SRb semi-regular variable star[24].
- W Vulpeculae's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.69'}[25].
- W Vulpeculae's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.24'}[26].
Body
Designation and Status
Recorded instance of include long-period variable star[2] and emission-line star[3].
History and Context
Catalog codes include GCRV 12522[6], GSC 02162-01244[7], HD 191652[8], HIC 99362[9], HIP 99362[10], and IRAS 20079+2608[11].