Scattering and sublimation: a multiscale view of µm-sized dust in the inclined disc of HD 145718 - Archive ouverte HAL Access content directly
Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2022

Scattering and sublimation: a multiscale view of µm-sized dust in the inclined disc of HD 145718

Claire L. Davies
  • Function : Author
Evan A. Rich
  • Function : Author
Tim J. Harries
  • Function : Author
John D. Monnier
  • Function : Author
Anna S. E. Laws
  • Function : Author
Sean M. Andrews
  • Function : Author
Jaehan Bae
  • Function : Author
David J. Wilner
  • Function : Author
Narsireddy Anugu
  • Function : Author
Jacob Ennis
  • Function : Author
Tyler Gardner
  • Function : Author
Stefan Kraus
  • Function : Author
Aaron Labdon
  • Function : Author
Cyprien Lanthermann
  • Function : Author
Gail H. Schaefer
  • Function : Author
Benjamin R. Setterholm
  • Function : Author
Theo ten Brummelaar
  • Function : Author

Abstract

We present multi-instrument observations of the disc around the Herbig Ae star, HD 145718, employing geometric and Monte Carlo radiative transfer models to explore the disc orientation, the vertical and radial extent of the near-infrared (NIR) scattering surface, and the properties of the dust in the disc surface and sublimation rim. The disc appears inclined at 67-71°, with position angle, PA = -1.0 to 0.6°, consistent with previous estimates. The NIR scattering surface extends out to ${\sim}75\,$ au and we infer an aspect ratio, hscat(r)/r ~ 0.24 in J band; ~0.22 in H band. Our Gemini Planet Imager images and VLTI + CHARA NIR interferometry suggest that the disc surface layers are populated by grains ≳λ/2π in size, indicating these grains are aerodynamically supported against settling and/or the density of smaller grains is relatively low. We demonstrate that our geometric analysis provides a reasonable assessment of the height of the NIR scattering surface at the outer edge of the disc and, if the inclination can be independently constrained, has the potential to probe the flaring exponent of the scattering surface in similarly inclined (i ≳ 70°) discs. In re-evaluating HD 145718's stellar properties, we found that the object's dimming events - previously characterized as UX Or and dipper variability - are consistent with dust occultation by grains larger, on average, than found in the ISM. This occulting dust likely originates close to the inferred dust sublimation radius at $0.17\,$ au.

Dates and versions

insu-03705355 , version 1 (27-06-2022)

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Claire L. Davies, Evan A. Rich, Tim J. Harries, John D. Monnier, Anna S. E. Laws, et al.. Scattering and sublimation: a multiscale view of µm-sized dust in the inclined disc of HD 145718. Monthly Notices of the Royal Astronomical Society, 2022, 511, pp.2434-2452. ⟨10.1093/mnras/stac149⟩. ⟨insu-03705355⟩
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