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WISE 0607+2429

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Star in the constellation Gemini


WISEP J060738.65+242953.4
Observation data
Epoch 2010.30      Equinox J2000
Constellation Gemini
Right ascension 06 07 38.65
Declination 24° 29′ 53.5″
Characteristics
Spectral type L8
Apparent magnitude (i) 20.02 ± 0.03
Apparent magnitude (z) 16.94 ± 0.01
Apparent magnitude (J (2MASS filter system)) 14.22 ± 0.03
Apparent magnitude (H (2MASS filter system)) 13.04 ± 0.03
Apparent magnitude (KS (2MASS filter system)) 12.47 ± 0.02
Astrometry
Proper motion (μ) RA: -472.871 mas/yr
Dec.: -318.464 mas/yr
Parallax (π)138.0616 ± 0.5185 mas
Distance23.62 ± 0.09 ly
(7.24 ± 0.03 pc)
Details
Mass0.03–0.072 M
Luminosity10 L
Temperature1460 ± 90 K
Other designations
WISEP J060738.65+242953.4
W0607+2429
2MASSW J06073908+2429574
2MASS J06073908+2429574
SDSS J060738.79+242954.4
Database references
SIMBADdata

WISEP J060738.65+242953.4 (designation is abbreviated to W0607+2429) is a brown dwarf of spectral class L8, located in the constellation Gemini at approximately 25 light-years from Earth.

Discovery

WISEP J060738.65+242953.4 was discovered in 2012 by Castro & Gizis from data collected by the Wide-field Infrared Survey Explorer (WISE) Earth-orbiting satelliteNASA infrared-wavelength 40 centimetres (16 in) space telescope, whose mission lasted from December 2009 to February 2011. There are also precovery identifications of this object in Two Micron All-Sky Survey (2MASS) data (observation epoch 1998.11) and in the Sloan Digital Sky Survey (SDSS) (DR7) (observation epoch 2006.98). In 2012 Castro & Gizis published a paper in The Astrophysical Journal, where they presented discovery of a newfound WISE L-type brown dwarf WISEP J060738.65+242953.4 (a single discovery, presented in the article).

Distance

Trigonometric parallax of WISEP J060738.65+242953.4 is not yet measured. Therefore, there are only distance estimates of this object, obtained by indirect — spectrophotometric — means (see table).

WISEP J060738.65+242953.4 distance estimates
Source Parallax, mas Distance, pc Distance, ly Ref.
Castro & Gizis (2012) 7.8
−1.2
25.4
−3.9
Gaia EDR3 138.0616 7.24±0.03 23.62±0.09

Non-trigonometric distance estimates are marked in italic.

Physical properties

WISEP J060738.65+242953.4 has a temperature of 1460 ± 90 K and bolometric luminosity of 10 Solar luminosities (the estimates are based on the object's spectral class (L8)). Mass estimates, determined from this temperature, are from 0.03 (for an assumed age of 0.5 Gyr) to 0.072 (for an assumed age of 10 Gyr) Solar masses, below the hydrogen-burning limit, which implies that WISEP J060738.65+242953.4 is not a true star, but only a substellar object.

While some researchers had claimed that WISEP J060738.65+242953.4 may be viewed from its pole, or may rotate slowly because of its narrow spectral lines, later work demonstrated that both of these claims were unlikely. This latter study estimated that the size of the radio-emitting magnetosphere is approximately 10 m.

See also

References

  1. ^ Castro, Philip J.; Gizis, John E. (2012). "Discovery of a Late L Dwarf: WISEP J060738.65+242953.4". The Astrophysical Journal. 746 (1): 3. arXiv:1110.4351. Bibcode:2012ApJ...746....3C. doi:10.1088/0004-637X/746/1/3. S2CID 119271171.
  2. ^ Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  3. "2MASS J06073908+2429574 -- Infrared source". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2012-12-24.
  4. ^ Gizis, John E.; Burgasser, Adam J.; Faherty, Jacqueline K.; Castro, Philip J.; Shara, Michael M. (2011). "WISEP J180026.60+013453.1: A nearby late-L Dwarf near the Galactic Plane". The Astronomical Journal. 142 (5): 171. arXiv:1109.0054. Bibcode:2011AJ....142..171G. doi:10.1088/0004-6256/142/5/171. S2CID 118596629.
  5. Route, Matthew (July 10, 2017). "Is WISEP J060738.65+242953.4 Really A Magnetically Active, Pole-on L Dwarf?". The Astrophysical Journal. 843 (2): 115. arXiv:1706.03010. Bibcode:2017ApJ...843..115R. doi:10.3847/1538-4357/aa78ab. S2CID 119056418.
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