V420 Aurigae

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V420 Aurigae

A light curve for V420 Aurigae, plotted from Hipparcos data[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga
Right ascension 05h 22m 35.23140s[2]
Declination +37° 40′ 33.6386″[2]
Apparent magnitude (V) 7.35 - 7.51[3]
Characteristics
Spectral type B0IVpe[4]
U−B color index −0.88[5]
B−V color index +0.16[5]
Variable type
Distance
4,500 ± 100 ly
(1,390 ± 40 pc)
Details
HD 34921 A
Rotational velocity (v sin i)
240±4[10] km/s
HIP 25114, SAO 57950[11]
Database references
SIMBADdata

V420 Aurigae is a high-mass

compact companion. Closely orbiting each other every 0.8 days, they are a source of X-ray emission.[6]

These coordinates were identified as an X-ray source using the

Balmer line emission, with these varying on a time scale of less than 300 seconds. This lends support to the presence of a compact companion.[13] The system displays an infrared excess, suggesting it has an orbiting circumstellar envelope of gas and possibly dust.[4] The system appears to be positioned at the center of an irregular, wispy nebula that was detected in the infrared band. One of the two filaments in this nebula appears to be connected with the system.[12]

References

  1. ^ "/ftp/cats/more/HIP/cdroms/cats". Centre de Données astronomiques de Strasbourg. Strasbourg astronomical Data Center. Retrieved 15 October 2022.
  2. ^
    S2CID 244398875
    . Gaia DR3 record for this source at VizieR.
  3. ^
    AAVSO
    , retrieved 2022-06-12
  4. ^ .
  5. ^ .
  6. ^ .
  7. .
  8. .
  9. .
  10. .
  11. ^ "HD 34921". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-11-10.
  12. ^
    S2CID 119443071
    , A37.
  13. .

Further reading

External links