Q74038596
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Q74038596
Summary
Q74038596 is a RS Canum Venaticorum variable[1].
Key Facts
- Q74038596's instance of is recorded as RS Canum Venaticorum variable[2].
- Q74038596's instance of is recorded as emission-line star[3].
- Q74038596's instance of is recorded as near-infrared source[4].
- Q74038596's instance of is recorded as variable star[5].
- Q74038596's instance of is recorded as astrophysical X-ray source[6].
- Q74038596's constellation is recorded as Perseus[7].
- Q74038596's spectral class is recorded as K1IV[8].
- Q74038596's catalog code is recorded as 2MASS J02521758+3616481[9].
- Q74038596's catalog code is recorded as 1RXS J025216.9+361658[10].
- Q74038596's catalog code is recorded as GSC 02338-00893[11].
- Q74038596's catalog code is recorded as UCAC2 44434062[12].
- Q74038596's catalog code is recorded as UCAC3 253-22471[13].
- Q74038596's catalog code is recorded as Gaia DR2 140684922252215552[14].
- Q74038596's catalog code is recorded as V875 Per[15].
- Q74038596's catalog code is recorded as TYC 2338-893-1[16].
- Q74038596's catalog code is recorded as TIC 67657567[17].
- Q74038596's catalog code is recorded as Gaia DR3 140684922252215552[18].
- Q74038596's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.59'}[19].
- Q74038596's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.83'}[20].
- Q74038596's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.449'}[21].
- Q74038596's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.794'}[22].
- Q74038596's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.602'}[23].
- Q74038596's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.37'}[24].
- Q74038596's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.44295'}[25].
- Q74038596's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.0665'}[26].
Body
Definition and Type
Recorded instance of include RS Canum Venaticorum variable[2], emission-line star[3], near-infrared source[4], variable star[5], and astrophysical X-ray source[6].