The VAST survey - IV. A wide brown dwarf companion to the A3V star ζ Delphini

R. J. De Rosa, J. Patience, K. Ward-Duong, A. Vigan, C. Marois, I. Song, B. Macintosh, J. R. Graham, R. Doyon, M. S. Bessel, O. Lai, Donald W Mccarthy, C. Kulesa

Research output: Contribution to journalArticle

14 Citations (Scopus)

Abstract

We report the discovery of a wide comoving substellar companion to the nearby (D = 67.5 ± 1.1 pc) A3V star ζ Delphini based on imaging and follow-up spectroscopic observations obtained during the course of our Volume-limited A-Star (VAST) multiplicity survey. ζ Del was observed over a five-year baseline with adaptive optics, revealing the presence of a previously unresolved companion with a proper motion consistent with that of the A-type primary. The age of the ζ Del system was estimated as 525 ± 125 Myr based on the position of the primary on the colour-magnitude and temperature-luminosity diagrams. Using intermediate-resolution near-infrared spectroscopy, the spectrum of ζ Del B is shown to be consistent with a mid-L dwarf (L5 ± 2), at a temperature of 1650 ± 200 K. Combining the measured near-infrared magnitude of ζ Del B with the estimated temperature leads to a modeldependent mass estimate of 50 ± 15MJup, corresponding to a mass ratio of q = 0.019 ± 0.006. At a projected separation of 910 ± 14 au, ζ Del B is among the most widely separated and extreme-mass ratio substellar companions to a main-sequence star resolved to date, providing a rare empirical constraint of the formation of low-mass ratio companions at extremely wide separations.

Original languageEnglish (US)
Pages (from-to)3694-3705
Number of pages12
JournalMonthly Notices of the Royal Astronomical Society
Volume445
Issue number4
DOIs
StatePublished - Sep 29 2014

Fingerprint

A stars
mass ratios
stars
near infrared
main sequence stars
proper motion
adaptive optics
temperature
infrared spectroscopy
diagrams
luminosity
color
diagram
estimates

Keywords

  • Binaries: visual
  • Brown dwarfs
  • Stars: early-type
  • Stars:individual: ζ Del
  • Techniques: high angular resolution
  • Techniques: spectroscopic

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

De Rosa, R. J., Patience, J., Ward-Duong, K., Vigan, A., Marois, C., Song, I., ... Kulesa, C. (2014). The VAST survey - IV. A wide brown dwarf companion to the A3V star ζ Delphini. Monthly Notices of the Royal Astronomical Society, 445(4), 3694-3705. https://doi.org/10.1093/mnras/stu2018

The VAST survey - IV. A wide brown dwarf companion to the A3V star ζ Delphini. / De Rosa, R. J.; Patience, J.; Ward-Duong, K.; Vigan, A.; Marois, C.; Song, I.; Macintosh, B.; Graham, J. R.; Doyon, R.; Bessel, M. S.; Lai, O.; Mccarthy, Donald W; Kulesa, C.

In: Monthly Notices of the Royal Astronomical Society, Vol. 445, No. 4, 29.09.2014, p. 3694-3705.

Research output: Contribution to journalArticle

De Rosa, RJ, Patience, J, Ward-Duong, K, Vigan, A, Marois, C, Song, I, Macintosh, B, Graham, JR, Doyon, R, Bessel, MS, Lai, O, Mccarthy, DW & Kulesa, C 2014, 'The VAST survey - IV. A wide brown dwarf companion to the A3V star ζ Delphini', Monthly Notices of the Royal Astronomical Society, vol. 445, no. 4, pp. 3694-3705. https://doi.org/10.1093/mnras/stu2018
De Rosa, R. J. ; Patience, J. ; Ward-Duong, K. ; Vigan, A. ; Marois, C. ; Song, I. ; Macintosh, B. ; Graham, J. R. ; Doyon, R. ; Bessel, M. S. ; Lai, O. ; Mccarthy, Donald W ; Kulesa, C. / The VAST survey - IV. A wide brown dwarf companion to the A3V star ζ Delphini. In: Monthly Notices of the Royal Astronomical Society. 2014 ; Vol. 445, No. 4. pp. 3694-3705.
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AU - De Rosa, R. J.

AU - Patience, J.

AU - Ward-Duong, K.

AU - Vigan, A.

AU - Marois, C.

AU - Song, I.

AU - Macintosh, B.

AU - Graham, J. R.

AU - Doyon, R.

AU - Bessel, M. S.

AU - Lai, O.

AU - Mccarthy, Donald W

AU - Kulesa, C.

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N2 - We report the discovery of a wide comoving substellar companion to the nearby (D = 67.5 ± 1.1 pc) A3V star ζ Delphini based on imaging and follow-up spectroscopic observations obtained during the course of our Volume-limited A-Star (VAST) multiplicity survey. ζ Del was observed over a five-year baseline with adaptive optics, revealing the presence of a previously unresolved companion with a proper motion consistent with that of the A-type primary. The age of the ζ Del system was estimated as 525 ± 125 Myr based on the position of the primary on the colour-magnitude and temperature-luminosity diagrams. Using intermediate-resolution near-infrared spectroscopy, the spectrum of ζ Del B is shown to be consistent with a mid-L dwarf (L5 ± 2), at a temperature of 1650 ± 200 K. Combining the measured near-infrared magnitude of ζ Del B with the estimated temperature leads to a modeldependent mass estimate of 50 ± 15MJup, corresponding to a mass ratio of q = 0.019 ± 0.006. At a projected separation of 910 ± 14 au, ζ Del B is among the most widely separated and extreme-mass ratio substellar companions to a main-sequence star resolved to date, providing a rare empirical constraint of the formation of low-mass ratio companions at extremely wide separations.

AB - We report the discovery of a wide comoving substellar companion to the nearby (D = 67.5 ± 1.1 pc) A3V star ζ Delphini based on imaging and follow-up spectroscopic observations obtained during the course of our Volume-limited A-Star (VAST) multiplicity survey. ζ Del was observed over a five-year baseline with adaptive optics, revealing the presence of a previously unresolved companion with a proper motion consistent with that of the A-type primary. The age of the ζ Del system was estimated as 525 ± 125 Myr based on the position of the primary on the colour-magnitude and temperature-luminosity diagrams. Using intermediate-resolution near-infrared spectroscopy, the spectrum of ζ Del B is shown to be consistent with a mid-L dwarf (L5 ± 2), at a temperature of 1650 ± 200 K. Combining the measured near-infrared magnitude of ζ Del B with the estimated temperature leads to a modeldependent mass estimate of 50 ± 15MJup, corresponding to a mass ratio of q = 0.019 ± 0.006. At a projected separation of 910 ± 14 au, ζ Del B is among the most widely separated and extreme-mass ratio substellar companions to a main-sequence star resolved to date, providing a rare empirical constraint of the formation of low-mass ratio companions at extremely wide separations.

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