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WISE 1800+0134

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(Redirected from WISEP J180026.60+013453.1) Brown dwarf in the constellation Ophiuchus
WISEP J180026.60+013453.1
Observation data
Epoch 2010.22      Equinox J2000
Constellation Ophiuchus
Right ascension 18 00 26.60
Declination 01° 34′ 53.1″
Characteristics
Spectral type L7.5
Apparent magnitude (J (2MASS filter system)) 14.30 ± 0.04
Apparent magnitude (H (2MASS filter system)) 13.12 ± 0.04
Apparent magnitude (KS (2MASS filter system)) 12.42 ± 0.03
Astrometry
Proper motion (μ) RA: 183.734 mas/yr
Dec.: -384.108 mas/yr
Parallax (π)128.0546 ± 0.5101 mas
Distance25.5 ± 0.1 ly
(7.81 ± 0.03 pc)
Details
Mass0.045±0.015 M
Luminosity10 L
Temperature1430 ± 100 K
Rotation9.3 hours
Rotational velocity (v sin i)13.5±0.5 km/s
Age0.9±0.6 Gyr
Other designations
WISEP J180026.60+013453.1
W1800+0134
2MASS J18002648+0134565
DENIS J180026.4+013457
DENIS-P J180026.4+013457
Database references
SIMBADdata
WISE 1800+0134 is located in 100x100WISE 1800+0134

WISEP J180026.60+013453.1 (designation is abbreviated to W1800+0134) is a brown dwarf of spectral class L7.5, located in constellation Ophiuchus at approximately 26 light-years from Earth.

Discovery

WISEP J180026.60+013453.1 was discovered in 2011 by Gizis et al. from data, collected by Wide-field Infrared Survey Explorer (WISE) Earth-orbiting satelliteNASA infrared-wavelength 40 centimetres (16 in)) space telescope, which mission lasted from December 2009 to February 2011. There are also precovery identifications of this object in Two Micron All-Sky Survey (2MASS) data (observed on 2000 September 23) and in the 3rd release of the DENIS database (close in time to the 2MASS observation). On 2011 June 22 Gizis et al. had conducted near-infrared spectroscopy with SpeX spectrograph, mounted on the 3 m Infrared Telescope Facility (IRTF), located at the Mauna Kea Observatory in Hawaii. In 2011 Gizis et al. published a paper in The Astronomical Journal, where they presented discovery of a newfound by WISE L-type brown dwarf WISEP J180026.60+013453.1 (a single discovery, presented in the article).

Physical properties

WISEP J180026.60+013453.1 has temperature 1430 ± 100 K and luminosity 10 Solar luminosities (the estimates are based on the object's spectral class (L7.5)). Mass estimates, determined from this temperature, are 0.04, 0.05, and 0.074 Solar masses, anyway below the hydrogen-burning limit, which implies that WISEP J180026.60+013453.1 is not a true star, but only a substellar object, that is a brown dwarf.

Failed test for binarity

WISEP J180026.60+013453.1 was tested spectroscopically for L + T binarity, and the binarity was not revealed. Common proper motion companions also were not found.

See also

Notes

  1. For an assumed age 0.5 Gyr.
  2. For an assumed age 1 Gyr.
  3. For an assumed age 5 Gyr.

References

  1. ^ 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.
  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. ^ Gizis, John E.; et al. (2015). "Properties of the Nearby Brown Dwarf WISEP J180026.60+013453.1". The Astronomical Journal. 150 (6). 179. arXiv:1509.04690. Bibcode:2015AJ....150..179G. doi:10.1088/0004-6256/150/6/179. S2CID 118641133.
  4. "WISEP J180026.60+013453.1 -- Brown Dwarf (M<0.08solMass)". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2012-12-24.
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