BERSIER , D.

Last name: BERSIER

First name: D.

2006 (v1)

Journal article

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

Nardetto, N. Mourard, D. Kervella, P.

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

Uploaded on: December 3, 2022
2004 (v1)

Journal article

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Cepheid distances from infrared long-baseline interferometry I. VINCI/VLTI observations of seven galactic cepheids

Kervella, P. Nardetto, N. Bersier, D.

Astronomy and Astrophysics, v. 416, p. 941-953, 2004. http://dx.doi.org/10.1051/0004-6361:20031743

Uploaded on: December 3, 2022
2004 (v1)

Journal article

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Cepheid distances from infrared long-baseline interferometry II. Calibration of the Period-Radius and Period-Luminosity relations

Kervella, P. Bersier, D. Mourard, D.

Astronomy and Astrophysics, v. 423, p. 327-333, 2004. http://dx.doi.org/10.1051/0004-6361:20035596

Uploaded on: December 3, 2022
2004 (v1)

Journal article

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Self consistent modelling of the projection factor for interferometric distance determination

Nardetto, N. Fokin, A. Mourard, D.

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

Uploaded on: December 3, 2022
September 2004 (v1)

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Cepheid pulsations resolved by the VLTI.

Kervella, P. Bersier, D. Nardetto, N.

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Uploaded on: February 27, 2023
April 4, 2005 (v1)

Conference paper

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Cepheid Distances from Interferometry

Kervella, P. Nardetto, N. Bersier, D.

Long baseline interferometry is now able to resolve the pulsational changes of the angular diameters of a significant number of Cepheids in the solar neighborhood. This allows us to apply a new version of the Baade-Wesselink method to measure their distances, for which we do not need to estimate the star?s temperature. Using this method and...

Uploaded on: December 4, 2022
December 2004 (v1)

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Cepheid distances from infrared long-baseline interferometry. III. Calibration of the surface brightness-color relations

Kervella, P. Bersier, D. Mourard, D.

The recent VINCI/VLTI observations presented in Paper I have nearly doubled the total number of available angular diameter measurements of Cepheids. Taking advantage of the significantly larger color range covered by these observations, we derive in the present paper high precision calibrations of the surface brightness-color relations using...

Uploaded on: December 4, 2022

BERSIER , D.

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