SwePub
Sök i LIBRIS databas

  Utökad sökning

id:"swepub:oai:DiVA.org:kth-305626"
 

Sökning: id:"swepub:oai:DiVA.org:kth-305626" > Brown dwarfs as ide...

Brown dwarfs as ideal candidates for detecting UV aurora outside the Solar System : Hubble Space Telescope observations of 2MASS J1237+6526

Saur, Joachim (författare)
Univ Cologne, Inst Geophys & Meteorol, Cologne, Germany.
Willmes, Clarissa (författare)
Univ Cologne, Inst Geophys & Meteorol, Cologne, Germany.
Fischer, Christian (författare)
Univ Cologne, Inst Geophys & Meteorol, Cologne, Germany.
visa fler...
Wennmacher, Alexandre (författare)
Univ Cologne, Inst Geophys & Meteorol, Cologne, Germany.
Roth, Lorenz (författare)
KTH,Rymd- och plasmafysik
Youngblood, Allison (författare)
Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80309 USA.
Strobel, Darrell F. (författare)
Johns Hopkins Univ, Dept Earth & Planetary Sci, Baltimore, MD 21218 USA.;Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA.
Reiners, Ansgar (författare)
Georg August Univ, Inst Astrophys, Gottingen, Germany.
visa färre...
Univ Cologne, Inst Geophys & Meteorol, Cologne, Germany Rymd- och plasmafysik (creator_code:org_t)
2021-11-22
2021
Engelska.
Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 655
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • Context. Observations of auroral emissions are powerful means to remotely sense the space plasma environment around planetary bodies and ultracool dwarfs. Therefore successful searches and characterization of aurorae outside the Solar System will open new avenues in the area of extrasolar space physics. Aims. We aim to demonstrate that brown dwarfs are ideal objects to search for UV aurora outside the Solar System. We specifically search for UV aurora on the late-type T6.5 brown dwarf 2MASS J12373919+6526148 (in the following 2MASS J1237+6526). Methods. Introducing a parameter referred to as auroral power potential, we derive scaling models for auroral powers for rotationally driven aurora applicable to a broad range of wavelengths. We also analyze Hubble Space Telescope observations obtained with the STIS camera at near-UV, far-UV, and Ly-alpha wavelengths of 2MASS J1237+6526. Results. We show that brown dwarfs, due to their typically strong surface magnetic fields and fast rotation, can produce auroral UV powers on the order of 10(19) watt or more. Considering their negligible thermal UV emission, their potentially powerful auroral emissions make brown dwarfs ideal candidates for detecting extrasolar aurorae. We find possible emission from 2MASS J1237+6526, but cannot conclusively attribute it to the brown dwarf due to low signal-to-noise values in combination with nonsystematic trends in the background fluxes. The observations provide upper limits for the emission at various UV wavelength bands. The upper limits for the emission correspond to a UV luminosity of similar to 1 x 10(19) watt, which lies in the range of the theoretically expected values. Conclusions. The possible auroral emission from the dwarf could be produced by a close-in companion and/or magnetospheric transport processes.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Nyckelord

brown dwarfs
planets and satellites: aurorae
ultraviolet: stars
ultraviolet: planetary systems
stars: individual: 2MASS J12373919+652614

Publikations- och innehållstyp

ref (ämneskategori)
art (ämneskategori)

Hitta via bibliotek

Till lärosätets databas

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Stäng

Kopiera och spara länken för att återkomma till aktuell vy