Kinematic distances of pre-main-sequence stars in the Lupus star-forming region
Idioma
en
Communication dans un congrès
Este ítem está publicado en
Proceedings of the International Astronomical Union, Advancing the Physics of Cosmic Distances, Proceedings of the International Astronomical Union, IAU Symposium, Volume 289, pp. 390-393, 2013, Advancing the Physics of Cosmic Distances, Proceedings of the International Astronomical Union, IAU Symposium, Volume 289, pp. 390-393, 2013, Advancing the Physics of Cosmic Distances, 2012, beijing. 2013-02, vol. 289, p. 390-393
Cambridge University Press (CUP)
Resumen en inglés
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 ...Leer más >
Palabras clave en inglés
stars: distances
stars: kinematics
stars: pre-main-sequence
ISM: individual (Lupus star-forming region)