Ask
Search
My library
ORKG

About
Statistics
Contact
Data Protection
Accessibility
Imprint
Changelog
Frontend: v1.32.0
Backend: v1.11.4

We use cookies to provide a better user experience.

Data Protection

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

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

Publication date

January 2007

DOI

10.1051/0004-6361:20066853

Publisher

EDP Sciences

Abstract

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

Extracted data

Related items

The projection factor, period–radius relation, and surface–brightness colour relation in classical cepheids

M. A. T. Groenewegen

October 2007

Context.The projection factor (p-factor) is of crucial importance in linking radial velocity variati...

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of

N. Nardetto
E. Poretti
M. Rainer
A. Fokin
P. Mathias
R. I. Anderson
A. Gallenne
W. Gieren
D. Graczyk
P. Kervella
A. Mérand
D. Mourard
H. Neilson
G. Pietrzynski
B. Pilecki
J. Storm

January 2017

Context. The projection factor p is the key quantity used in the Baade-Wesselink (BW) method for dis...

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...

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...

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...

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...

High-resolution spectroscopy for Cepheids distance determination

N. Nardetto
W. Gieren
P. Kervella
P. Fouqué
J. Storm
G. Pietrzynski
D. Mourard
D. Queloz

June 2009

Context. The cross correlation method (hereafter CC) is widely used to derive the radial velocity cu...

High-resolution spectroscopy for Cepheids distance determination

N. Nardetto
W. Gieren
P. Kervella
P. Fouqué
J. Storm
G. Pietrzynski
D. Mourard
D. Queloz

June 2009

Context. The cross correlation method (hereafter CC) is widely used to derive the radial velocity cu...

Self consistent modelling of the projection factor for interferometric distance determination

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

January 2004

Astronomy and Astrophysics, v. 428, p. 131-137, 2004. http://dx.doi.org/10.1051/0004-6361:20041419In...

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...

Observational calibration of the projection factor of Cepheids

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

March 2015

Context. The distance of pulsating stars, in particular Cepheids, are commonly measured using the pa...

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of δ Cep revisited

Nardetto, N.
Poretti, E.
Rainer, M.
Fokin, A.
Mathias, P.
Anderson, R.
Gallenne, A.
Gieren, W.
Graczyk, D.
Kervella, P.
Mérand, A.
Mourard, D.
Neilson, H.
Pietrzynski, G.
Pilecki, B.
Storm, J.

January 2017

International audienceContext. The projection factor p is the key quantity used in the Baade-Wesseli...

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of δ Cep revisited

Nardetto, N.
Poretti, E.
Rainer, M.
Fokin, A.
Mathias, P.
Anderson, R.
Gallenne, A.
Gieren, W.
Graczyk, D.
Kervella, P.
Mérand, A.
Mourard, D.
Neilson, H.
Pietrzynski, G.
Pilecki, B.
Storm, J.

January 2017

International audienceContext. The projection factor p is the key quantity used in the Baade-Wesseli...

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of δ Cep revisited

Nardetto, N.
Poretti, E.
Rainer, M.
Fokin, A.
Mathias, P.
Anderson, R.
Gallenne, A.
Gieren, W.
Graczyk, D.
Kervella, P.
Mérand, A.
Mourard, D.
Neilson, H.
Pietrzynski, G.
Pilecki, B.
Storm, J.

January 2017

International audienceContext. The projection factor p is the key quantity used in the Baade-Wesseli...

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of δ Cep revisited

Nardetto, N.
Poretti, E.
Rainer, M.
Fokin, A.
Mathias, P.
Anderson, R.
Gallenne, A.
Gieren, W.
Graczyk, D.
Kervella, P.
Mérand, A.
Mourard, D.
Neilson, H.
Pietrzynski, G.
Pilecki, B.
Storm, J.

January 2017

International audienceContext. The projection factor p is the key quantity used in the Baade-Wesseli...

The projection factor, period–radius relation, and surface–brightness colour relation in classical cepheids

M. A. T. Groenewegen

October 2007

Context.The projection factor (p-factor) is of crucial importance in linking radial velocity variati...

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of

N. Nardetto
E. Poretti
M. Rainer
A. Fokin
P. Mathias
R. I. Anderson
A. Gallenne
W. Gieren
D. Graczyk
P. Kervella
A. Mérand
D. Mourard
H. Neilson
G. Pietrzynski
B. Pilecki
J. Storm

January 2017

Context. The projection factor p is the key quantity used in the Baade-Wesselink (BW) method for dis...

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...

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...

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...

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...

High-resolution spectroscopy for Cepheids distance determination

N. Nardetto
W. Gieren
P. Kervella
P. Fouqué
J. Storm
G. Pietrzynski
D. Mourard
D. Queloz

June 2009

Context. The cross correlation method (hereafter CC) is widely used to derive the radial velocity cu...

High-resolution spectroscopy for Cepheids distance determination

N. Nardetto
W. Gieren
P. Kervella
P. Fouqué
J. Storm
G. Pietrzynski
D. Mourard
D. Queloz

June 2009

Context. The cross correlation method (hereafter CC) is widely used to derive the radial velocity cu...

Self consistent modelling of the projection factor for interferometric distance determination

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

January 2004

Astronomy and Astrophysics, v. 428, p. 131-137, 2004. http://dx.doi.org/10.1051/0004-6361:20041419In...

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...

Observational calibration of the projection factor of Cepheids

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

March 2015

Context. The distance of pulsating stars, in particular Cepheids, are commonly measured using the pa...

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of δ Cep revisited

Nardetto, N.
Poretti, E.
Rainer, M.
Fokin, A.
Mathias, P.
Anderson, R.
Gallenne, A.
Gieren, W.
Graczyk, D.
Kervella, P.
Mérand, A.
Mourard, D.
Neilson, H.
Pietrzynski, G.
Pilecki, B.
Storm, J.

January 2017

International audienceContext. The projection factor p is the key quantity used in the Baade-Wesseli...

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of δ Cep revisited

Nardetto, N.
Poretti, E.
Rainer, M.
Fokin, A.
Mathias, P.
Anderson, R.
Gallenne, A.
Gieren, W.
Graczyk, D.
Kervella, P.
Mérand, A.
Mourard, D.
Neilson, H.
Pietrzynski, G.
Pilecki, B.
Storm, J.

January 2017

International audienceContext. The projection factor p is the key quantity used in the Baade-Wesseli...

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of δ Cep revisited

Nardetto, N.
Poretti, E.
Rainer, M.
Fokin, A.
Mathias, P.
Anderson, R.
Gallenne, A.
Gieren, W.
Graczyk, D.
Kervella, P.
Mérand, A.
Mourard, D.
Neilson, H.
Pietrzynski, G.
Pilecki, B.
Storm, J.

January 2017

International audienceContext. The projection factor p is the key quantity used in the Baade-Wesseli...

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of δ Cep revisited

Nardetto, N.
Poretti, E.
Rainer, M.
Fokin, A.
Mathias, P.
Anderson, R.
Gallenne, A.
Gieren, W.
Graczyk, D.
Kervella, P.
Mérand, A.
Mourard, D.
Neilson, H.
Pietrzynski, G.
Pilecki, B.
Storm, J.

January 2017

International audienceContext. The projection factor p is the key quantity used in the Baade-Wesseli...

The projection factor, period–radius relation, and surface–brightness colour relation in classical cepheids

M. A. T. Groenewegen

October 2007

Context.The projection factor (p-factor) is of crucial importance in linking radial velocity variati...

HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of

N. Nardetto
E. Poretti
M. Rainer
A. Fokin
P. Mathias
R. I. Anderson
A. Gallenne
W. Gieren
D. Graczyk
P. Kervella
A. Mérand
D. Mourard
H. Neilson
G. Pietrzynski
B. Pilecki
J. Storm

January 2017

Context. The projection factor p is the key quantity used in the Baade-Wesselink (BW) method for dis...

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...