Q81792620
classical Cepheid variable star in the constellation Puppis
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Q81792620
Summary
Q81792620 is a classical Cepheid variable[1].
Key Facts
- Q81792620's instance of is recorded as classical Cepheid variable[2].
- Q81792620's instance of is recorded as Cepheid variable[3].
- Q81792620's instance of is recorded as near-infrared source[4].
- Q81792620's constellation is recorded as Puppis[5].
- Q81792620's catalog code is recorded as GSC 06562-00429[6].
- Q81792620's catalog code is recorded as NSV 3842[7].
- Q81792620's catalog code is recorded as 2MASS J07591220-2641560[8].
- Q81792620's catalog code is recorded as ASAS J075912-2641.9[9].
- Q81792620's catalog code is recorded as Gaia DR2 5601254523607154816[10].
- Q81792620's catalog code is recorded as V622 Pup[11].
- Q81792620's catalog code is recorded as OGLE GD1567.30.00014[12].
- Q81792620's catalog code is recorded as OGLE GD-CEP-157[13].
- Q81792620's catalog code is recorded as TIC 130269777[14].
- Q81792620's catalog code is recorded as UCAC4 317-037258[15].
- Q81792620's catalog code is recorded as Gaia DR3 5601254523607154816[16].
- Q81792620's type of variable star is recorded as classical Cepheid variable[17].
- Q81792620's type of variable star is recorded as Cepheid variable[18].
- Q81792620's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.824'}[19].
- Q81792620's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.404'}[20].
- Q81792620's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.221'}[21].
- Q81792620's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.735744'}[22].
- Q81792620's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.157'}[23].
- Q81792620's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.89'}[24].
- Q81792620's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.746'}[25].
- Q81792620's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.267'}[26].
Body
Definition and Type
Recorded instance of include classical Cepheid variable[2], Cepheid variable[3], and near-infrared source[4].