SwePub
Tyck till om SwePub Sök här!
Sök i LIBRIS databas

  Extended search

WFRF:(Brandner Wolfgang)
 

Search: WFRF:(Brandner Wolfgang) > (2019) > Schlieder Joshua > A search for variab...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

A search for variability in exoplanet analogues and low-gravity brown dwarfs

Vos, Johanna M. (author)
Biller, Beth A. (author)
Bonavita, Mariangela (author)
show more...
Eriksson, Simon (author)
Stockholms universitet,Institutionen för astronomi
Liu, Michael C. (author)
Best, William M. J. (author)
Metchev, Stanimir (author)
Radigan, Jacqueline (author)
Allers, Katelyn N. (author)
Janson, Markus (author)
Stockholms universitet,Institutionen för astronomi
Buenzli, Esther (author)
Dupuy, Trent J. (author)
Bonnefoy, Mickael (author)
Manjavacas, Elena (author)
Brandner, Wolfgang (author)
Crossfield, Ian (author)
Deacon, Niall (author)
Henning, Thomas (author)
Homeier, Derek (author)
Kopytova, Taisiya (author)
Schlieder, Joshua (author)
show less...
 (creator_code:org_t)
2018-11-22
2019
English.
In: Monthly notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 483:1, s. 480-502
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We report the results of a J-band survey for photometric variability in a sample of young, low-gravity objects using the New Technology Telescope (NTT) and the United Kingdom Infrared Telescope (UKIRT). Surface gravity is a key parameter in the atmospheric properties of brown dwarfs and this is the first large survey that aims to test the gravity dependence of variability properties. We do a full analysis of the spectral signatures of youth and assess the group membership probability of each target using membership tools from the literature. This results in a 30 object sample of young low-gravity brown dwarfs. Since we are lacking in objects with spectral types later than L9, we focus our statistical analysis on the L0-L8.5 objects. We find that the variability occurrence rate of L0-L8.5 low-gravity brown dwarfs in this survey is 30(-8)(+16) per cent. We reanalyse the results of Radigan (2014) and find that the field dwarfs with spectral types L0-L8.5 have a variability occurrence rate of 11(-4)(+13) per cent. We determine a probability of 98 per cent that the samples are drawn from different distributions. This is the first quantitative indication that the low-gravity objects are more likely to be variable than the field dwarf population. Furthermore, we present follow-up J(S) and K-S observations of the young, planetary-mass variable object PSO 318.5-22 over three consecutive nights. We find no evidence of phase shifts between the J(S) and K-S bands and find higher J(S) amplitudes. We use the J(S) light curves to measure a rotational period of 8.45 +/- 0.05 h for PSO 318.5-22.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

brown dwarfs
stars: variables: general

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

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 Close

Copy and save the link in order to return to this view