Self consistent modelling of the projection factor for interferometric distance determination

High-resolution spectroscopy for Cepheids distance determination

N. Nardetto
D. Mourard
Ph. Mathias
A. Fokin
D. Gillet

June 2007

Context.The projection factor is a key quantity for the interferometric Baade-Wesselink (hereafter I...

c © ESO 2005 Astronomy &Astrophysics The projection factor of δ Cephei A calibration of the Baade-Wesselink method using the CHARA Array

A. Mér
P. Kervella
V. Coudé Du Foresto
S. T. Ridgway
J. P. Aufdenberg
T. A. Ten Brummelaar
D. H. Berger
J. Sturmann
L. Sturmann
N. H. Turner
H. A. Mcalister

January 2005

Abstract. Cepheids play a key role in astronomy as standard candles for measuring intergalactic dist...

Observational calibration of the projection factor of Cepheids: IV. Period-projection factor relation of Galactic and Magellanic Cloud Cepheids

Gallenne, A.
Kervella, P.
Mérand, A.
Pietrzyński, G.
Gieren, W.
Nardetto, N.
Trahin, B.

December 2017

International audienceContext. The Baade-Wesselink (BW) method, which combines linear and angular di...

Self consistent modelling of the projection factor for interferometric distance determination

N. Nardetto
A. Fokin
D. Mourard
Ph. Mathias
P. Kervella
D. Bersier

November 2004

The distance of galactic Cepheids can be derived through the interferometric Baade-Wesselink method....

Self consistent modelling of the projection factor for interferometric distance determination

N. Nardetto
A. Fokin
D. Mourard
Ph. Mathias
P. Kervella
D. Bersier

November 2004

The distance of galactic Cepheids can be derived through the interferometric Baade-Wesselink method....

High-resolution spectroscopy for Cepheids distance determination - II. A period-projection factor relation

Nardetto, N.
Mourard, D.
Mathias, Ph.
Fokin, A.
Gillet, D.

January 2007

Astronomy and Astrophysics, v. 471, p. 661-669, 2007. http://dx.doi.org/10.1051/0004-6361:20066853In...

Observational calibration of the projection factor of Cepheids

J. Breitfelder
A. Mérand
P. Kervella
A. Gallenne
L. Szabados
R. I. Anderson
J.-B. Le Bouquin

February 2016

Context. The distance to pulsating stars is classically estimated using the parallax-of-pulsation (P...

The projection factor of delta Cephei A calibration of the Baade-Wesselink method using the CHARA Array

Antoine, Mérand
Kervella, Pierre
Coude Du Foresto, Vincent
T. Ridgway, Stephen
P. Aufdenberg, Jason
A. Ten Brummelaar, Theo
H. Berger, David
Sturmann, Judit
Sturmann, Laszlo
H. Turner, Nils
A. Mcalister, Harold

June 2005

6 pages (including an electronic table), accepted for publication in A&A lettersCepheids play a key ...

The projection factor of delta Cephei A calibration of the Baade-Wesselink method using the CHARA Array

Antoine, Mérand
Kervella, Pierre
Coude Du Foresto, Vincent
T. Ridgway, Stephen
P. Aufdenberg, Jason
A. Ten Brummelaar, Theo
H. Berger, David
Sturmann, Judit
Sturmann, Laszlo
H. Turner, Nils
A. Mcalister, Harold

June 2005

6 pages (including an electronic table), accepted for publication in A&A lettersCepheids play a key ...

The projection factor of delta Cephei A calibration of the Baade-Wesselink method using the CHARA Array

Antoine, Mérand
Kervella, Pierre
Coude Du Foresto, Vincent
T. Ridgway, Stephen
P. Aufdenberg, Jason
A. Ten Brummelaar, Theo
H. Berger, David
Sturmann, Judit
Sturmann, Laszlo
H. Turner, Nils
A. Mcalister, Harold

June 2005

6 pages (including an electronic table), accepted for publication in A&A lettersCepheids play a key ...

La dynamique atmosphérique des Céphéides et l'étalonnage des échelles de distance dans l'Univers

Nardetto, Nicolas

November 2005

Applying the Interferometric Baade-Wesselink method, hereafter IBW method, toVINCI/VLTI observations...

Observational calibration of the projection factor of Cepheids

Pierre Kervella
Boris Trahin
Howard E. Bond
Alexandre Gallenne
Laszlo Szabados
Antoine Mérand
Joanne Breitfelder
Julien Dailloux
Richard I. Anderson
Pascal Fouqué
Wolfgang Gieren
Nicolas Nardetto
Grzegorz Pietrzyński

April 2017

The projection factor (p-factor) is an essential component of the classical Baade-Wesselink (BW) tec...

High resolution spectroscopy for Cepheids distance determination: I. Line asymmetry

Nardetto, N.
Mourard, D.
Kervella, P.
Mathias, Ph.
Merand, A.
Bersier, D.

January 2006

Astronomy and Astrophysics, v. 453, p. 309-319, 2006. http://dx.doi.org/10.1051/0004-6361:20054333In...

Observational calibration of the projection factor of Cepheids II. Application to nine Cepheids with HST/FGS parallax measurements

Breitfelder, J.
Mérand, A.
Kervella, Pierre
Gallenne, A.
Szabados, L.
Anderson, R. I.
Le Bouquin, J.-B.

March 2016

Context. The distance to pulsating stars is classically estimated using the parallax-of-pulsation (P...

Calibrating the projection factor for Galactic Cepheids

C.-C. Ngeow
H. R. Neilson
N. Nardetto
M. Marengo

June 2012

Context. The projection factor (p), which converts the radial velocity to pulsational velocity, is a...

High-resolution spectroscopy for Cepheids distance determination

N. Nardetto
D. Mourard
Ph. Mathias
A. Fokin
D. Gillet

June 2007

Context.The projection factor is a key quantity for the interferometric Baade-Wesselink (hereafter I...

c © ESO 2005 Astronomy &Astrophysics The projection factor of δ Cephei A calibration of the Baade-Wesselink method using the CHARA Array

A. Mér
P. Kervella
V. Coudé Du Foresto
S. T. Ridgway
J. P. Aufdenberg
T. A. Ten Brummelaar
D. H. Berger
J. Sturmann
L. Sturmann
N. H. Turner
H. A. Mcalister

January 2005

Abstract. Cepheids play a key role in astronomy as standard candles for measuring intergalactic dist...

Observational calibration of the projection factor of Cepheids: IV. Period-projection factor relation of Galactic and Magellanic Cloud Cepheids

Gallenne, A.
Kervella, P.
Mérand, A.
Pietrzyński, G.
Gieren, W.
Nardetto, N.
Trahin, B.

December 2017

International audienceContext. The Baade-Wesselink (BW) method, which combines linear and angular di...

Self consistent modelling of the projection factor for interferometric distance determination

N. Nardetto
A. Fokin
D. Mourard
Ph. Mathias
P. Kervella
D. Bersier

November 2004

The distance of galactic Cepheids can be derived through the interferometric Baade-Wesselink method....

Self consistent modelling of the projection factor for interferometric distance determination

N. Nardetto
A. Fokin
D. Mourard
Ph. Mathias
P. Kervella
D. Bersier

November 2004

The distance of galactic Cepheids can be derived through the interferometric Baade-Wesselink method....

High-resolution spectroscopy for Cepheids distance determination - II. A period-projection factor relation

Nardetto, N.
Mourard, D.
Mathias, Ph.
Fokin, A.
Gillet, D.

January 2007

Astronomy and Astrophysics, v. 471, p. 661-669, 2007. http://dx.doi.org/10.1051/0004-6361:20066853In...

Observational calibration of the projection factor of Cepheids

J. Breitfelder
A. Mérand
P. Kervella
A. Gallenne
L. Szabados
R. I. Anderson
J.-B. Le Bouquin

February 2016

Context. The distance to pulsating stars is classically estimated using the parallax-of-pulsation (P...

The projection factor of delta Cephei A calibration of the Baade-Wesselink method using the CHARA Array

Antoine, Mérand
Kervella, Pierre
Coude Du Foresto, Vincent
T. Ridgway, Stephen
P. Aufdenberg, Jason
A. Ten Brummelaar, Theo
H. Berger, David
Sturmann, Judit
Sturmann, Laszlo
H. Turner, Nils
A. Mcalister, Harold

June 2005

6 pages (including an electronic table), accepted for publication in A&A lettersCepheids play a key ...

The projection factor of delta Cephei A calibration of the Baade-Wesselink method using the CHARA Array

Antoine, Mérand
Kervella, Pierre
Coude Du Foresto, Vincent
T. Ridgway, Stephen
P. Aufdenberg, Jason
A. Ten Brummelaar, Theo
H. Berger, David
Sturmann, Judit
Sturmann, Laszlo
H. Turner, Nils
A. Mcalister, Harold

June 2005

6 pages (including an electronic table), accepted for publication in A&A lettersCepheids play a key ...

The projection factor of delta Cephei A calibration of the Baade-Wesselink method using the CHARA Array

Antoine, Mérand
Kervella, Pierre
Coude Du Foresto, Vincent
T. Ridgway, Stephen
P. Aufdenberg, Jason
A. Ten Brummelaar, Theo
H. Berger, David
Sturmann, Judit
Sturmann, Laszlo
H. Turner, Nils
A. Mcalister, Harold

June 2005

6 pages (including an electronic table), accepted for publication in A&A lettersCepheids play a key ...

La dynamique atmosphérique des Céphéides et l'étalonnage des échelles de distance dans l'Univers

Nardetto, Nicolas

November 2005

Applying the Interferometric Baade-Wesselink method, hereafter IBW method, toVINCI/VLTI observations...

Observational calibration of the projection factor of Cepheids

Pierre Kervella
Boris Trahin
Howard E. Bond
Alexandre Gallenne
Laszlo Szabados
Antoine Mérand
Joanne Breitfelder
Julien Dailloux
Richard I. Anderson
Pascal Fouqué
Wolfgang Gieren
Nicolas Nardetto
Grzegorz Pietrzyński

April 2017

The projection factor (p-factor) is an essential component of the classical Baade-Wesselink (BW) tec...

High resolution spectroscopy for Cepheids distance determination: I. Line asymmetry

Nardetto, N.
Mourard, D.
Kervella, P.
Mathias, Ph.
Merand, A.
Bersier, D.

January 2006

Astronomy and Astrophysics, v. 453, p. 309-319, 2006. http://dx.doi.org/10.1051/0004-6361:20054333In...

Observational calibration of the projection factor of Cepheids II. Application to nine Cepheids with HST/FGS parallax measurements

Breitfelder, J.
Mérand, A.
Kervella, Pierre
Gallenne, A.
Szabados, L.
Anderson, R. I.
Le Bouquin, J.-B.

March 2016

Context. The distance to pulsating stars is classically estimated using the parallax-of-pulsation (P...

Calibrating the projection factor for Galactic Cepheids

C.-C. Ngeow
H. R. Neilson
N. Nardetto
M. Marengo

June 2012

Context. The projection factor (p), which converts the radial velocity to pulsational velocity, is a...

High-resolution spectroscopy for Cepheids distance determination

N. Nardetto
D. Mourard
Ph. Mathias
A. Fokin
D. Gillet

June 2007

Context.The projection factor is a key quantity for the interferometric Baade-Wesselink (hereafter I...

c © ESO 2005 Astronomy &Astrophysics The projection factor of δ Cephei A calibration of the Baade-Wesselink method using the CHARA Array

A. Mér
P. Kervella
V. Coudé Du Foresto
S. T. Ridgway
J. P. Aufdenberg
T. A. Ten Brummelaar
D. H. Berger
J. Sturmann
L. Sturmann
N. H. Turner
H. A. Mcalister

January 2005

Abstract. Cepheids play a key role in astronomy as standard candles for measuring intergalactic dist...

Observational calibration of the projection factor of Cepheids: IV. Period-projection factor relation of Galactic and Magellanic Cloud Cepheids

Gallenne, A.
Kervella, P.
Mérand, A.
Pietrzyński, G.
Gieren, W.
Nardetto, N.
Trahin, B.

December 2017

International audienceContext. The Baade-Wesselink (BW) method, which combines linear and angular di...

Self consistent modelling of the projection factor for interferometric distance determination

Abstract

Extracted data

Self consistent modelling of the projection factor for interferometric distance determination

Abstract

Extracted data

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