Commentary on the paper "The H-R Diagrams of Young Clusters and the Formation of Planetary Systems" by Poveda (1965)

Details Commentary on the paper "The H-R Diagrams of Young Clusters and the Formation of Planetary Systems" by Poveda (1965) Commentary on the paper "The H-R Diagrams of Young Clusters and the Formation of Planetary Systems" by Poveda (1965)

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..39...83r&link_type=abstract

Highlights of the Boletín de los Observatorios de Tonantzintla y Tacubaya (Eds. S. Torres-Peimbert & O. López-Cruz) Revista Mexi

Astronomy and Astrophysics

Astronomy

Herbig-Haro Objects, Ism: Jets And Outflows, Stars: Formation, Stars: Pre-Main Sequence

Scientific paper

I present a review on the paper by A. Poveda, 1965, BOTT, 4, 26, 15, where he discusses from a theoretical point of view the expected characteristics of a forming star. Originally motivated to explain two apparent puzzles of star formation, the existence of young stars below the main sequence and the Faulkner-Griffiths-Hoyle paradox, the paper went on to predict phenomena that were later confirmed observationally and that constitute important part of our present knowledge of stellar and planetary formation.

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