Q83839416
Press Enter · cited answer in seconds
0 sources
Q83839416
Summary
Q83839416 is an astrophysical X-ray source[1].
Key Facts
- Q83839416's instance of is recorded as astrophysical X-ray source[2].
- Q83839416's instance of is recorded as high proper-motion star[3].
- Q83839416's constellation is recorded as Centaurus[4].
- Q83839416's spectral class is recorded as G2V[5].
- Q83839416's catalog code is recorded as 1RXS J141624.4-522506[6].
- Q83839416's catalog code is recorded as CCDM J14164-5225AB[7].
- Q83839416's catalog code is recorded as CD-51 8084[8].
- Q83839416's catalog code is recorded as CPC 19 5396[9].
- Q83839416's catalog code is recorded as CPD-51 6721[10].
- Q83839416's catalog code is recorded as GSC 08289-00232[11].
- Q83839416's catalog code is recorded as HD 124670[12].
- Q83839416's catalog code is recorded as HIC 69736[13].
- Q83839416's catalog code is recorded as HIP 69736[14].
- Q83839416's catalog code is recorded as IDS 14097-5157 AB[15].
- Q83839416's catalog code is recorded as PPM 342698[16].
- Q83839416's catalog code is recorded as SAO 241584[17].
- Q83839416's catalog code is recorded as TYC 8289-232-1[18].
- Q83839416's catalog code is recorded as WDS J14164-5225AB[19].
- Q83839416's catalog code is recorded as Gaia DR2 5897344213180223872[20].
- Q83839416's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.63'}[21].
- Q83839416's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.26'}[22].
- Q83839416's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.5236'}[23].
- Q83839416's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+9.3501'}[24].
- Q83839416's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+2.63'}[25].
- Q83839416's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+106.9507'}[26].
Body
Definition and Type
Recorded instance of include astrophysical X-ray source[2] and high proper-motion star[3].