Cool customers in the stellar graveyard. II. Limits to substellar objects around nearby DAZ white dwarfs

John H. Debes, Steinn Sigurdsson, Bruce E. Woodgate

Research output: Contribution to journalReview article

18 Citations (Scopus)

Abstract

Results from a concerted Hubble Space Telescope (HST) survey of nearby white dwarfs for substellar objects are presented. A total of seven DAZ white dwarfs with distances of <50 pc had high-contrast and high spatial resolution NICMOS coronagraphic images taken to search for candidate substellar objects at separations ≲10″ away. Limits to unresolved companions are derived through analysis of Two Micron All Sky Survey photometry of the white dwarfs compared to expected fluxes based on the white dwarf's effective temperature, distance, and gravity. Our HST survey of seven DAZ white dwarfs identified candidate companions for four of the white dwarfs. For three of these, HST and ground-based second-epoch observations showed the candidates to be background stars. The fourth white dwarf, which is close to the Galactic plane, has seven candidate companions at distances of 2″-4″, which remain to be followed up. We find that for four of the white dwarfs we are sensitive to planetary companions of ≳M J. For all the targets, we are sensitive to companions of >18M J. The lack of significant near-IR excesses for our targets limits any kind of unresolved companions present to be substellar. In light of these results we make several comments on the possibility of determining the origin of metals in the atmospheres of these white dwarfs.

Original languageEnglish (US)
Pages (from-to)1221-1230
Number of pages10
JournalAstronomical Journal
Volume130
Issue number3
DOIs
StatePublished - Sep 1 2005

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Hubble Space Telescope
atmospheres
atmosphere
metal
metals

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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title = "Cool customers in the stellar graveyard. II. Limits to substellar objects around nearby DAZ white dwarfs",
abstract = "Results from a concerted Hubble Space Telescope (HST) survey of nearby white dwarfs for substellar objects are presented. A total of seven DAZ white dwarfs with distances of <50 pc had high-contrast and high spatial resolution NICMOS coronagraphic images taken to search for candidate substellar objects at separations ≲10″ away. Limits to unresolved companions are derived through analysis of Two Micron All Sky Survey photometry of the white dwarfs compared to expected fluxes based on the white dwarf's effective temperature, distance, and gravity. Our HST survey of seven DAZ white dwarfs identified candidate companions for four of the white dwarfs. For three of these, HST and ground-based second-epoch observations showed the candidates to be background stars. The fourth white dwarf, which is close to the Galactic plane, has seven candidate companions at distances of 2″-4″, which remain to be followed up. We find that for four of the white dwarfs we are sensitive to planetary companions of ≳M J. For all the targets, we are sensitive to companions of >18M J. The lack of significant near-IR excesses for our targets limits any kind of unresolved companions present to be substellar. In light of these results we make several comments on the possibility of determining the origin of metals in the atmospheres of these white dwarfs.",
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Cool customers in the stellar graveyard. II. Limits to substellar objects around nearby DAZ white dwarfs. / Debes, John H.; Sigurdsson, Steinn; Woodgate, Bruce E.

In: Astronomical Journal, Vol. 130, No. 3, 01.09.2005, p. 1221-1230.

Research output: Contribution to journalReview article

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AB - Results from a concerted Hubble Space Telescope (HST) survey of nearby white dwarfs for substellar objects are presented. A total of seven DAZ white dwarfs with distances of <50 pc had high-contrast and high spatial resolution NICMOS coronagraphic images taken to search for candidate substellar objects at separations ≲10″ away. Limits to unresolved companions are derived through analysis of Two Micron All Sky Survey photometry of the white dwarfs compared to expected fluxes based on the white dwarf's effective temperature, distance, and gravity. Our HST survey of seven DAZ white dwarfs identified candidate companions for four of the white dwarfs. For three of these, HST and ground-based second-epoch observations showed the candidates to be background stars. The fourth white dwarf, which is close to the Galactic plane, has seven candidate companions at distances of 2″-4″, which remain to be followed up. We find that for four of the white dwarfs we are sensitive to planetary companions of ≳M J. For all the targets, we are sensitive to companions of >18M J. The lack of significant near-IR excesses for our targets limits any kind of unresolved companions present to be substellar. In light of these results we make several comments on the possibility of determining the origin of metals in the atmospheres of these white dwarfs.

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