Toward a renewed Galactic Cepheid distance scale from Gaia and optical interferometry

Pierre Kervella, Antoine Mérand, Alexandre Gallenne, Boris Trahin, Nicolas Nardetto, Richard I. Anderson, Joanne Breitfelder, Laszlo Szabados, Howard E. Bond, Simon Borgniet, Wolfgang Gieren, Grzegorz Pietrzyński

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Through an innovative combination of multiple observing techniques and modeling, we are assembling a comprehensive understanding of the pulsation and close environment of Cepheids. We developed the SPIPS modeling tool that combines all observables (radial velocimetry, photometry, angular diameters from interferometry) to derive the relevant physical parameters of the star (effective temperature, infrared excess, reddening, ⋯) and the ratio of the distance and the projection factor d/p. We present the application of SPIPS to the long-period Cepheid RS Pup, for which we derive p = 1.25±0.06. The addition of this massive Cepheid consolidates the existing sample of p-factor measurements towards long-period pulsators. This allows us to conclude that p is constant or mildly variable around p = 1.29±0.04 (±3%) as a function of the pulsation period. The forthcoming Gaia DR2 will provide a considerable improvement in quantity and accuracy of the trigonometric parallaxes of Cepheids. From this sample, the SPIPS modeling tool will enable a robust calibration of the Cepheid distance scale.

Original languageEnglish (US)
Title of host publicationWide-Field Variability Surveys
Subtitle of host publicationA 21st Century Perspective - 22nd Los Alamos Stellar Pulsation - Conference Series Meeting
EditorsWolfgang Gieren, Marcio Catelan, Wolfgang Gieren, Marcio Catelan
PublisherEDP Sciences
ISBN (Electronic)9782759890248
DOIs
StatePublished - Sep 8 2017
Event22nd Los Alamos Stellar Pulsation Conference Series Meeting 2016 - San Pedro de Atacama, Chile
Duration: Nov 28 2016Dec 2 2016

Publication series

NameEPJ Web of Conferences
Volume152
ISSN (Print)2101-6275
ISSN (Electronic)2100-014X

Other

Other22nd Los Alamos Stellar Pulsation Conference Series Meeting 2016
CountryChile
CitySan Pedro de Atacama
Period11/28/1612/2/16

Fingerprint

interferometry
assembling
photometry
projection
stars
temperature

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Cite this

Kervella, P., Mérand, A., Gallenne, A., Trahin, B., Nardetto, N., Anderson, R. I., ... Pietrzyński, G. (2017). Toward a renewed Galactic Cepheid distance scale from Gaia and optical interferometry. In W. Gieren, M. Catelan, W. Gieren, & M. Catelan (Eds.), Wide-Field Variability Surveys: A 21st Century Perspective - 22nd Los Alamos Stellar Pulsation - Conference Series Meeting [07003] (EPJ Web of Conferences; Vol. 152). EDP Sciences. https://doi.org/10.1051/epjconf/201715207002
Kervella, Pierre ; Mérand, Antoine ; Gallenne, Alexandre ; Trahin, Boris ; Nardetto, Nicolas ; Anderson, Richard I. ; Breitfelder, Joanne ; Szabados, Laszlo ; Bond, Howard E. ; Borgniet, Simon ; Gieren, Wolfgang ; Pietrzyński, Grzegorz. / Toward a renewed Galactic Cepheid distance scale from Gaia and optical interferometry. Wide-Field Variability Surveys: A 21st Century Perspective - 22nd Los Alamos Stellar Pulsation - Conference Series Meeting. editor / Wolfgang Gieren ; Marcio Catelan ; Wolfgang Gieren ; Marcio Catelan. EDP Sciences, 2017. (EPJ Web of Conferences).
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abstract = "Through an innovative combination of multiple observing techniques and modeling, we are assembling a comprehensive understanding of the pulsation and close environment of Cepheids. We developed the SPIPS modeling tool that combines all observables (radial velocimetry, photometry, angular diameters from interferometry) to derive the relevant physical parameters of the star (effective temperature, infrared excess, reddening, ⋯) and the ratio of the distance and the projection factor d/p. We present the application of SPIPS to the long-period Cepheid RS Pup, for which we derive p = 1.25±0.06. The addition of this massive Cepheid consolidates the existing sample of p-factor measurements towards long-period pulsators. This allows us to conclude that p is constant or mildly variable around p = 1.29±0.04 (±3{\%}) as a function of the pulsation period. The forthcoming Gaia DR2 will provide a considerable improvement in quantity and accuracy of the trigonometric parallaxes of Cepheids. From this sample, the SPIPS modeling tool will enable a robust calibration of the Cepheid distance scale.",
author = "Pierre Kervella and Antoine M{\'e}rand and Alexandre Gallenne and Boris Trahin and Nicolas Nardetto and Anderson, {Richard I.} and Joanne Breitfelder and Laszlo Szabados and Bond, {Howard E.} and Simon Borgniet and Wolfgang Gieren and Grzegorz Pietrzyński",
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Kervella, P, Mérand, A, Gallenne, A, Trahin, B, Nardetto, N, Anderson, RI, Breitfelder, J, Szabados, L, Bond, HE, Borgniet, S, Gieren, W & Pietrzyński, G 2017, Toward a renewed Galactic Cepheid distance scale from Gaia and optical interferometry. in W Gieren, M Catelan, W Gieren & M Catelan (eds), Wide-Field Variability Surveys: A 21st Century Perspective - 22nd Los Alamos Stellar Pulsation - Conference Series Meeting., 07003, EPJ Web of Conferences, vol. 152, EDP Sciences, 22nd Los Alamos Stellar Pulsation Conference Series Meeting 2016, San Pedro de Atacama, Chile, 11/28/16. https://doi.org/10.1051/epjconf/201715207002

Toward a renewed Galactic Cepheid distance scale from Gaia and optical interferometry. / Kervella, Pierre; Mérand, Antoine; Gallenne, Alexandre; Trahin, Boris; Nardetto, Nicolas; Anderson, Richard I.; Breitfelder, Joanne; Szabados, Laszlo; Bond, Howard E.; Borgniet, Simon; Gieren, Wolfgang; Pietrzyński, Grzegorz.

Wide-Field Variability Surveys: A 21st Century Perspective - 22nd Los Alamos Stellar Pulsation - Conference Series Meeting. ed. / Wolfgang Gieren; Marcio Catelan; Wolfgang Gieren; Marcio Catelan. EDP Sciences, 2017. 07003 (EPJ Web of Conferences; Vol. 152).

Research output: Chapter in Book/Report/Conference proceedingConference contribution

TY - GEN

T1 - Toward a renewed Galactic Cepheid distance scale from Gaia and optical interferometry

AU - Kervella, Pierre

AU - Mérand, Antoine

AU - Gallenne, Alexandre

AU - Trahin, Boris

AU - Nardetto, Nicolas

AU - Anderson, Richard I.

AU - Breitfelder, Joanne

AU - Szabados, Laszlo

AU - Bond, Howard E.

AU - Borgniet, Simon

AU - Gieren, Wolfgang

AU - Pietrzyński, Grzegorz

PY - 2017/9/8

Y1 - 2017/9/8

N2 - Through an innovative combination of multiple observing techniques and modeling, we are assembling a comprehensive understanding of the pulsation and close environment of Cepheids. We developed the SPIPS modeling tool that combines all observables (radial velocimetry, photometry, angular diameters from interferometry) to derive the relevant physical parameters of the star (effective temperature, infrared excess, reddening, ⋯) and the ratio of the distance and the projection factor d/p. We present the application of SPIPS to the long-period Cepheid RS Pup, for which we derive p = 1.25±0.06. The addition of this massive Cepheid consolidates the existing sample of p-factor measurements towards long-period pulsators. This allows us to conclude that p is constant or mildly variable around p = 1.29±0.04 (±3%) as a function of the pulsation period. The forthcoming Gaia DR2 will provide a considerable improvement in quantity and accuracy of the trigonometric parallaxes of Cepheids. From this sample, the SPIPS modeling tool will enable a robust calibration of the Cepheid distance scale.

AB - Through an innovative combination of multiple observing techniques and modeling, we are assembling a comprehensive understanding of the pulsation and close environment of Cepheids. We developed the SPIPS modeling tool that combines all observables (radial velocimetry, photometry, angular diameters from interferometry) to derive the relevant physical parameters of the star (effective temperature, infrared excess, reddening, ⋯) and the ratio of the distance and the projection factor d/p. We present the application of SPIPS to the long-period Cepheid RS Pup, for which we derive p = 1.25±0.06. The addition of this massive Cepheid consolidates the existing sample of p-factor measurements towards long-period pulsators. This allows us to conclude that p is constant or mildly variable around p = 1.29±0.04 (±3%) as a function of the pulsation period. The forthcoming Gaia DR2 will provide a considerable improvement in quantity and accuracy of the trigonometric parallaxes of Cepheids. From this sample, the SPIPS modeling tool will enable a robust calibration of the Cepheid distance scale.

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U2 - 10.1051/epjconf/201715207002

DO - 10.1051/epjconf/201715207002

M3 - Conference contribution

T3 - EPJ Web of Conferences

BT - Wide-Field Variability Surveys

A2 - Gieren, Wolfgang

A2 - Catelan, Marcio

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A2 - Catelan, Marcio

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Kervella P, Mérand A, Gallenne A, Trahin B, Nardetto N, Anderson RI et al. Toward a renewed Galactic Cepheid distance scale from Gaia and optical interferometry. In Gieren W, Catelan M, Gieren W, Catelan M, editors, Wide-Field Variability Surveys: A 21st Century Perspective - 22nd Los Alamos Stellar Pulsation - Conference Series Meeting. EDP Sciences. 2017. 07003. (EPJ Web of Conferences). https://doi.org/10.1051/epjconf/201715207002