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Kinematic distances of pre-main-sequence stars in the Lupus star-forming region
(International Astronomical UnionBeijing, 2012)
To reliably determine the main physical parameters (masses and ages) of young stars, we must know their distances. While the average distance to nearby star-forming regions (<300 pc) is often known, the distances to ...
Kinematic distances of pre-main-sequence stars in the Lupus star-forming region
(International Astronomical UnionBeijing, 2012)
To reliably determine the main physical parameters (masses and ages) of young stars, we must know their distances. While the average distance to nearby star-forming regions (<300 pc) is often known, the distances to ...
The DR14 APOGEE-TGAS catalogue: Precise chemo-kinematics in the extended solar vicinity
(Cambridge University Press, 2017)
Trigonometric parallaxes in the TW Hydrae Association
(International Astronomical UnionBeijing, 2012)
We have conducted a program of trigonometric distance measurements to 13 members of the TW Hydrae Association (TWA), which will enable us (through back-tracking methods) to derive a convincing estimate of the age of the ...
Trigonometric parallaxes in the TW Hydrae Association
(International Astronomical UnionBeijing, 2012)
We have conducted a program of trigonometric distance measurements to 13 members of the TW Hydrae Association (TWA), which will enable us (through back-tracking methods) to derive a convincing estimate of the age of the ...
Calibrating the surface brightness – color relation for late-type red giants stars in the visible domain using VEGA/CHARA interferometric observations
(EDP Science, 2020)
Context. The surface brightness - color relationship (SBCR) is a poweful tool for determining the angular diameter of stars from photometry. It was for instance used to derive the distance of eclipsing binaries in the Large ...