Q80477014
young stellar object in the constellation Ophiuchus
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Q80477014
Summary
Q80477014 is a young stellar object[1].
Key Facts
- Q80477014's instance of is recorded as young stellar object[2].
- Q80477014's constellation is recorded as Ophiuchus[3].
- Q80477014's spectral class is recorded as K5Ve[4].
- Q80477014 is part of Scorpius–Centaurus Association[5].
- Q80477014's catalog code is recorded as CD-27 11535[6].
- Q80477014's catalog code is recorded as CPD-27 5600[7].
- Q80477014's catalog code is recorded as GSC 06820-00223[8].
- Q80477014's catalog code is recorded as PPM 733155[9].
- Q80477014's catalog code is recorded as TYC 6820-223-1[10].
- Q80477014's catalog code is recorded as 2MASS J17150362-2749397[11].
- Q80477014's catalog code is recorded as 1RXS J171503.2-274934[12].
- Q80477014's catalog code is recorded as ASAS J171503-2749.5[13].
- Q80477014's catalog code is recorded as [SZB2012] 93[14].
- Q80477014's catalog code is recorded as Gaia DR1 4107812481173239680[15].
- Q80477014's catalog code is recorded as Gaia DR2 4107812485571331328[16].
- Q80477014's type of variable star is recorded as rotating variable star[17].
- Q80477014's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.174'}[18].
- Q80477014's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.537'}[19].
- Q80477014's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.384'}[20].
- Q80477014's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.68'}[21].
- Q80477014's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.129'}[22].
- Q80477014's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.596'}[23].
- Q80477014's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.0315'}[24].
- Q80477014's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+12.0040'}[25].
- Q80477014's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.33'}[26].
Body
Definition and Type
Q80477014's instance of is recorded as young stellar object[2].
Use and Application
Q80477014 is part of Scorpius–Centaurus Association[5].