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词条 DENIS J082303.1-491201
释义

  1. History

  2. References

{{Starbox begin}}{{Starbox observe
|epoch=J2000
|constell=Vela
|ra={{RA|08|23|03.13}}[1]
|dec={{DEC|-49|12|01.3}}[1]
|appmag_v=
}}{{Starbox character
|appmag_1_passband=R
|appmag_1=20.020[2]
|class=L1.5 + L5.5[3]
}}{{Starbox astrometry
|prop_mo_ra=−154.92[3]
|prop_mo_dec=7.99[3]
|dist_pc=20.69 ± 0.06[3]
|dist_ly={{cvt|20.69|±|0.06|pc|ly|disp=number}}
}}{{Starbox orbit
|reference=[4]
|period_unitless=247.75 ± 0.64 d
|axis=4.62 ± 0.12 mas
|inclination=52.2 ± 1.5
|node=346.2 ± 2.0
|periastron=JD 2455927.323928
|eccentricity=0.36 ± 0.04
|periarg=41.8 ± 4.7
}}{{Starbox detail
|source=[3]
|component1=A
|mass=0.028−0.063
|temperature=2150 ± 100
|luminosity=0.00018
|age_myr=80–500
|component2=B
|mass2=0.018−0.045
|temperature2=1670 ± 140
|luminosity2=0.000063
}}{{Starbox catalog
|names={{odlist|2MASS=J08230313-4912012}}[2]
}}{{Starbox reference
|Simbad=2MASS+J08230313-4912012
}}{{Starbox end}}

DENIS-P J082303.1-491201 (also known as DENIS J082303.1-491201, DE0823-49), is a binary system of two brown dwarfs, located {{convert|20.77|pc|ly}} away from the Earth. The system is located in the constellation Vela.

The primary has a spectral class of L1.5, a mass of {{solar mass|0.028 to 0.063}} and a temperature of {{convert|2150|K|C F}}. The secondary is also a brown dwarf but with a spectral type of L5.5, a mass of {{solar mass|0.018 to 0.045}}, and a temperature of {{convert|1670|K|C F}}. The mass ratio is around 0.64 to 0.74.[3]

The system has an orbital period of 248 days. The age of the system is estimated to be around 80 to 500 millions years old, a relatively young object in the solar neighbourhood, however it does not seem to belong to have any association with any moving groups.[3]

History

DENIS J082303.1-491201 was discovered by Ngoc Phan-Bao et al as part of the Deep Near Infrared Survey of the Southern Sky or DENIS for short.[5]

Detected in 2006, DE0823-49 b was included in the NASA Exoplanet Archive as the first exoplanet discovered by the Astrometry exoplanet detection method.[6][7]

References

1. ^{{cite journal|title=2MASS All-Sky Catalog of Point Sources|date=2003|journal=VizieR On-line Data Catalog|author=Cutri, R. M.|display-authors=etal|bibcode=2003yCat.2246....0C}}
2. ^{{cite simbad|title=2MASS J08230313-4912012|accessdate=19 September 2017}}
3. ^{{cite journal|doi=10.1051/0004-6361/201425536|title=DE0823−49 is a juvenile binary brown dwarf at 20.7 pc|arxiv=1505.07972|bibcode=2015A&A...579A..61S}}
4. ^{{cite web|url=http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/orb6|title=Sixth Catalog of Orbits of Visual Binary Stars|publisher=United States Naval Observatory|accessdate=19 September 2017}}
5. ^{{cite journal|first=Ngoc|last=Phan-Bao|author-link=|display-authors=etal|title=Discovery of new nearby L and late-M dwarfs at low Galactic latitude from the DENIS data base|publisher=Monthly Notices of the Royal Astronomical Society|volume=383|number=3|date=January 2008|pages=831–844|doi=10.1111/j.1365-2966.2007.12564.x|bibcode=2008MNRAS.383..831P|arxiv=0708.4169|url=http://cdsads.u-strasbg.fr/cgi-bin/nph-iarticle_query?2008MNRAS.383..831P&classic=YES|format=gif|access-date=1 June 2015 }}.
6. ^{{cite web|title=Exoplanet and candidate statistics|url=http://exoplanetarchive.ipac.caltech.edu/docs/counts_detail.html|work=NASA Exoplanet Archive|accessdate=1 June 2015}}
7. ^{{cite web|title=Liste des exoplanètes découvertes par astrométrie|url=http://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=planets&constraint=pl_discmethod+like+%27Astrometry%25%27|work=NASA Exoplanet Archive|accessdate=1 June 2015}}
{{Stars of Vela}}

5 : Brown dwarfs|L-type stars|Binary stars|2MASS objects|Vela (constellation)

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