Combined spectroscopy and intensity interferometry to determine the distances of the blue supergiants P Cygni and Rigel - Archive ouverte HAL Access content directly
Journal Articles Monthly Notices of the Royal Astronomical Society: Letters Year : 2022

Combined spectroscopy and intensity interferometry to determine the distances of the blue supergiants P Cygni and Rigel

(1) , (2) , (1) , (1) , (1) , (2) , (2) , , (2) , (1) , (3) , (2) , (2)
1
2
3
E. S. G. de Almeida
Mathilde Hugbart
Armando Domiciano de Souza
  • Function : Author
  • PersonId : 996152
Jean-Pierre Rivet
Antonin Siciak
  • Function : Author
  • PersonId : 1081420
Guillaume Labeyrie
  • Function : Author
  • PersonId : 1112283
Olivier Garde
  • Function : Author
Nolan Matthews
  • Function : Author
  • PersonId : 1130754
Olivier Lai
David Vernet
  • Function : Author
  • PersonId : 1037945
Robin Kaiser
William Guerin

Abstract

In this paper we report on spatial intensity interferometry measurements within the H$\alpha$ line on two stars: the Luminous Blue Variable supergiant P Cygni, and the late-type B supergiant Rigel. The experimental setup was upgraded to allow simultaneous measurement of two polarization channels, instead of one in our previous setup, and the zero baseline correlation function on-sky to validate independent estimates obtained from the stellar spectrum and the instrumental spectral throughput. Combined with simultaneous spectra measurements and based on radiative transfer models calculated with the code CMFGEN, we were able to fit our measured visibility curves to extract the stellar distances. Our distance determinations for both P Cygni (1.61 ± 0.18 kpc) and Rigel (0.26 ± 0.02 kpc) agree very well with the values provided by astrometry with the Gaia and Hipparcos missions, respectively. This result for Rigel was obtained by adopting a stellar luminosity of Lstar = 123000 Lsun, which is reported in the literature as being consistent with the Hipparcos distance to Rigel. However, due to the lack of consensus on Rigel's luminosity, we also explore how the adoption of the stellar luminosity in our models affects our distance determination for Rigel. In conclusion, we support, in an independent way, the distance to Rigel as the one provided by the Hipparcos mission, when taking the luminosity of 123000 Lsun at face value. This study is the first successful step towards extending the application of the Wind Momentum Luminosity Relation method for distance calibration from an LBV supergiant to a more normal late-type B supergiant.
Fichier principal
Vignette du fichier
main.pdf (1.78 Mo) Télécharger le fichier
Origin : Files produced by the author(s)

Dates and versions

hal-03615887 , version 1 (22-03-2022)
hal-03615887 , version 2 (20-06-2022)

Identifiers

Cite

E. S. G. de Almeida, Mathilde Hugbart, Armando Domiciano de Souza, Jean-Pierre Rivet, Farrokh Vakili, et al.. Combined spectroscopy and intensity interferometry to determine the distances of the blue supergiants P Cygni and Rigel. Monthly Notices of the Royal Astronomical Society: Letters, 2022, 515, pp.1-12. ⟨10.1093/mnras/stac1617⟩. ⟨hal-03615887v2⟩
604 View
26 Download

Altmetric

Share

Gmail Facebook Twitter LinkedIn More