Keck LWS images of the compact nebula around RY Scuti in the thermal infrared

Robert D. Gehrz, Nathan Smith, Barbara Jones, Richard Puetter, Amos Yahil

Research output: Contribution to journalArticle

23 Citations (Scopus)

Abstract

We report new 3 to 20 μm Keck Telescope images of the massive eclipsing binary RY Scuti with ∼0″.25 spatial resolution. These images show complex structure near the diffraction limit of the 10 m telescope in a nebula less than 2″ across. The limb-brightened structure is consistent with optically thin emission from a circumstellar torus. At 3 to 5 μm, the extended emission is predominantly scattered photospheric light from the central stars. The 8.9, 11.7, 12.5, and 18.7 μm images are dominated by thermal emission from warm carbon and silicate dust in the outer regions of the torus. The new observations are consistent with the geometric models previously proposed by Gehrz et al. and Smith et al. to explain the structures observed in the circumstellar environment of RY Scuti. For example, the inside of the torus is ionized by the central star and shows strong emission from [Ne II] at 12.8 μm. Double-ring structure similar to that seen in Hubble Space Telescope images is partly resolved at the limb-brightened edges of the torus in the new mid-infrared continuum images, and the new IR images are consistent with two parallel dust rings adjacent to the ionized gas rings and farther from the star. The new mid-infrared images at 8.9, 11.7, and 12.5 μm show faint emission from a thin disk outside the previously detected torus. We estimate a dust mass in the torus of 1.4 × 10-6 M⊙ and a neon abundance in the ionized gas of nNe/nH ≳ 1.77 × 10-4 from the 12.8 μm [Ne II] emission.

Original languageEnglish (US)
Pages (from-to)395-401
Number of pages7
JournalAstrophysical Journal
Volume559
Issue number1 PART 1
DOIs
StatePublished - Sep 20 2001
Externally publishedYes

Fingerprint

nebulae
dust
ionized gases
limbs
stars
limb
telescopes
neon
rings
ring structures
thermal emission
Hubble Space Telescope
gas
diffraction
silicates
spatial resolution
silicate
continuums
carbon
estimates

Keywords

  • Binaries: eclipsing
  • Circumstellar matter
  • Infrared: stars
  • Stars: individual (RY Scuti)
  • Stars: mass loss
  • Stars: winds, outflows

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Keck LWS images of the compact nebula around RY Scuti in the thermal infrared. / Gehrz, Robert D.; Smith, Nathan; Jones, Barbara; Puetter, Richard; Yahil, Amos.

In: Astrophysical Journal, Vol. 559, No. 1 PART 1, 20.09.2001, p. 395-401.

Research output: Contribution to journalArticle

Gehrz, RD, Smith, N, Jones, B, Puetter, R & Yahil, A 2001, 'Keck LWS images of the compact nebula around RY Scuti in the thermal infrared', Astrophysical Journal, vol. 559, no. 1 PART 1, pp. 395-401. https://doi.org/10.1086/322325
Gehrz, Robert D. ; Smith, Nathan ; Jones, Barbara ; Puetter, Richard ; Yahil, Amos. / Keck LWS images of the compact nebula around RY Scuti in the thermal infrared. In: Astrophysical Journal. 2001 ; Vol. 559, No. 1 PART 1. pp. 395-401.
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