Astronomy and Astrophysics, v. 453, p. 309-319, 2006. http://dx.doi.org/10.1051/0004-6361:20054333International audienc
Comments : 9 pages, 3 Postscript figures, 5 Tables, accepted for publication in A&AInternational aud...
4 pages, 4 figuresLong baseline interferometry is now able to resolve the pulsational change of the ...
4 pages, 4 figuresLong baseline interferometry is now able to resolve the pulsational change of the ...
Astronomy and Astrophysics, v. 471, p. 661-669, 2007. http://dx.doi.org/10.1051/0004-6361:20066853In...
Context.The ratio of pulsation to radial velocity (the projection factor) is currently limiting the ...
Context.The ratio of pulsation to radial velocity (the projection factor) is currently limiting the ...
Context. Galactic Cepheids in the vicinity of the Sun have a residual line-of-sight velocity, or γ-v...
Context. The cross correlation method (hereafter CC) is widely used to derive the radial velocity cu...
Context. The cross correlation method (hereafter CC) is widely used to derive the radial velocity cu...
Context. Galactic Cepheids in the vicinity of the Sun have a residual line-of-sight velocity, or gam...
Context. Galactic Cepheids in the vicinity of the Sun have a residual line-of-sight velocity, or gam...
Applying the Interferometric Baade-Wesselink method, hereafter IBW method, toVINCI/VLTI observations...
Context. In recent years, infrared interferometry has revealed the presence of faint dusty circumste...
Context.The projection factor is a key quantity for the interferometric Baade-Wesselink (hereafter I...
Context.The projection factor is a key quantity for the interferometric Baade-Wesselink (hereafter I...
Comments : 9 pages, 3 Postscript figures, 5 Tables, accepted for publication in A&AInternational aud...
4 pages, 4 figuresLong baseline interferometry is now able to resolve the pulsational change of the ...
4 pages, 4 figuresLong baseline interferometry is now able to resolve the pulsational change of the ...
Astronomy and Astrophysics, v. 471, p. 661-669, 2007. http://dx.doi.org/10.1051/0004-6361:20066853In...
Context.The ratio of pulsation to radial velocity (the projection factor) is currently limiting the ...
Context.The ratio of pulsation to radial velocity (the projection factor) is currently limiting the ...
Context. Galactic Cepheids in the vicinity of the Sun have a residual line-of-sight velocity, or γ-v...
Context. The cross correlation method (hereafter CC) is widely used to derive the radial velocity cu...
Context. The cross correlation method (hereafter CC) is widely used to derive the radial velocity cu...
Context. Galactic Cepheids in the vicinity of the Sun have a residual line-of-sight velocity, or gam...
Context. Galactic Cepheids in the vicinity of the Sun have a residual line-of-sight velocity, or gam...
Applying the Interferometric Baade-Wesselink method, hereafter IBW method, toVINCI/VLTI observations...
Context. In recent years, infrared interferometry has revealed the presence of faint dusty circumste...
Context.The projection factor is a key quantity for the interferometric Baade-Wesselink (hereafter I...
Context.The projection factor is a key quantity for the interferometric Baade-Wesselink (hereafter I...
Comments : 9 pages, 3 Postscript figures, 5 Tables, accepted for publication in A&AInternational aud...
4 pages, 4 figuresLong baseline interferometry is now able to resolve the pulsational change of the ...
4 pages, 4 figuresLong baseline interferometry is now able to resolve the pulsational change of the ...
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