Q66611870
astrophysical X-ray source in the constellation Scorpius
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Q66611870
Summary
Q66611870 is a high proper-motion star[1].
Key Facts
- Q66611870's instance of is recorded as high proper-motion star[2].
- Q66611870's instance of is recorded as astrophysical X-ray source[3].
- Q66611870's constellation is recorded as Scorpius[4].
- Q66611870's spectral class is recorded as F3V[5].
- Q66611870's catalog code is recorded as HD 162763[6].
- Q66611870's catalog code is recorded as CPC 18 9074[7].
- Q66611870's catalog code is recorded as GSC 07886-01385[8].
- Q66611870's catalog code is recorded as HIC 87665[9].
- Q66611870's catalog code is recorded as HIP 87665[10].
- Q66611870's catalog code is recorded as 2MASS J17542438-3837352[11].
- Q66611870's catalog code is recorded as PPM 296978[12].
- Q66611870's catalog code is recorded as SAO 209439[13].
- Q66611870's catalog code is recorded as uvby98 100162763[14].
- Q66611870's catalog code is recorded as TYC 7886-1385-1[15].
- Q66611870's catalog code is recorded as Gaia DR1 4036773584662950784[16].
- Q66611870's catalog code is recorded as Gaia DR2 4036773589046451584[17].
- Q66611870's catalog code is recorded as 1RXS J175423.4-383743[18].
- Q66611870's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.63'}[19].
- Q66611870's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.19'}[20].
- Q66611870's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.0758'}[21].
- Q66611870's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.332'}[22].
- Q66611870's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.133'}[23].
- Q66611870's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.116'}[24].
- Q66611870's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+18.2217'}[25].
- Q66611870's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-4.78'}[26].
Body
Definition and Type
Recorded instance of include high proper-motion star[2] and astrophysical X-ray source[3].