Q78244122
W Ursae Majoris variable star in the constellation Orion
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Q78244122
Summary
Q78244122 is a young stellar object[1].
Key Facts
- Q78244122's instance of is recorded as young stellar object[2].
- Q78244122's instance of is recorded as eclipsing binary star[3].
- Q78244122's instance of is recorded as near-infrared source[4].
- Q78244122's instance of is recorded as astrophysical X-ray source[5].
- Q78244122's constellation is recorded as Orion[6].
- Q78244122's spectral class is recorded as M5[7].
- Q78244122's catalog code is recorded as 2MASS J05352568-0530381[8].
- Q78244122's catalog code is recorded as CSV 6273[9].
- Q78244122's catalog code is recorded as NSV 2327[10].
- Q78244122's catalog code is recorded as [AD95] 568[11].
- Q78244122's catalog code is recorded as [DRS2009] 500[12].
- Q78244122's catalog code is recorded as [MGM2012] 1534[13].
- Q78244122's catalog code is recorded as Gaia DR2 3017359012449387136[14].
- Q78244122's catalog code is recorded as V1537 Ori[15].
- Q78244122's catalog code is recorded as TIC 427395412[16].
- Q78244122's catalog code is recorded as Gaia DR3 3017359012449387136[17].
- Q78244122's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.947'}[18].
- Q78244122's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.030'}[19].
- Q78244122's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.877'}[20].
- Q78244122's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.394'}[21].
- Q78244122's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.53'}[22].
- Q78244122's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.034'}[23].
- Q78244122's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.948602'}[24].
- Q78244122's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.4733'}[25].
- Q78244122's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+26.5475'}[26].
Body
Definition and Type
Recorded instance of include young stellar object[2], eclipsing binary star[3], near-infrared source[4], and astrophysical X-ray source[5].