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词条 WISE J031624.35+430709.1
释义

  1. Discovery

  2. Distance

  3. References

{{Sky|03|16|24.35|+|43|07|09.1|106.3}}{{Starbox begin
|name=WISE J031624.35+430709.1}}{{Starbox observe
|epoch=J2000{{r|Kirkpatrick2012}}
|equinox=J2000{{r|Kirkpatrick2012}}
|constell=Perseus
|ra={{RA|03|16|24.35}}{{r|Kirkpatrick2012}}
|dec={{DEC|43|07|09.1}}{{r|Kirkpatrick2012}}}}{{Starbox character
|class=T8{{r|Kirkpatrick2012}}
|appmag_3_passband=H
|appmag_3=19.70 ± 0.09{{r|Kirkpatrick2012}}
}}{{Starbox astrometry
|dist_pc=~ 32.6{{r|Kirkpatrick2012}}
|dist_ly=~ 106.3{{r|Kirkpatrick2012}}}}{{Starbox catalog
|names=WISE J031624.35+430709.1{{r|Kirkpatrick2012}}}}{{Starbox end}}

WISE J031624.35+430709.1 is a brown dwarf of spectral class T8,{{r|Kirkpatrick2012}} located in constellation Perseus at approximately 106 light-years from Earth.{{r|Kirkpatrick2012}} It is one of the furthest T-class brown dwarfs known.

Discovery

WISE J031624.35+430709.1 was discovered in 2012 by Mace et al. from data, collected by Wide-field Infrared Survey Explorer (WISE) Earth-orbiting satellite — NASA infrared-wavelength 40 cm (16 in) space telescope, which mission lasted from December 2009 to February 2011. In March 2013, the discovery paper was published.{{r|Mace2013}}

Distance

Trigonometric parallax of WISE J031624.35+430709.1 is not yet measured. Therefore, there are only distance estimates of this object, obtained by indirect — spectrofotometric — means (see table).

WISE J031624.35+430709.1 distance estimates
Source Parallax, mas Distance, pc Distance, ly Ref.
Kirkpatrick et al. (2012), Table 8 32.6 106.3 Kirkpatrick2012}}
Non-trigonometric distance estimates are marked in italic.

References

1. ^{{cite journal|last1=Mace|first1=Gregory N.|last2=Kirkpatrick|first2=J. Davy|last3=Cushing|first3=Michael C.|last4=Gelino|first4=Christopher R.|last5=Griffith |first5=Roger L.|last6=Skrutskie|first6=Michael F.|last7=Marsh|first7=Kenneth A.|last8=Wright |first8=Edward L.|last9=Eisenhardt|first9=Peter R.|last10=McLean|first10=Ian S.| last11=Thompson|first11=Maggie A.|last12=mix|first12=Katholeen|last13=Bailey| first13=Vanessa|last14=Beichman|first14=Charles A.|last15=Bloom|first15=Joshua S. |last16=Burgasser|first16=Adam J.|last17=Fortney|first17=Jonathan J.|last18=Hinz |first18=Philip M.|last19=Knox|first19=Russell P.|last20=Lowrance|first20=Patrick J.|last21=Marley|first21=Mark S.|last22=Morley|first22=Caroline V.|last23=Rodigas |first23=Timothy J.|last24=Saumon|first24=Didier|last25=Sheppard|first25=Scott S.|last26=Stock |first26=Nathan D.|year=2013|title=A Study of the Diverse T Dwarf Population Revealed by WISE|journal=The Astrophysical Journal Supplement Series|volume=205|issue=6|pages=1–49 |doi=10.1088/0067-0049/205/1/6|arxiv = 1301.3913 |bibcode = 2013ApJS..205....6M }}
[1]
}}{{Stars of Perseus}}{{Brown-dwarf-stub}}

4 : Brown dwarfs|T-type stars|Perseus (constellation)|WISE objects

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