O curso fornece uma introdução à formação de estrelas focada na pré-sequência principal (estrelas de baixa massa e de massa intermediária). Os tópicos começam na escala galáctica, diminuindo até as escalas de estrelas individuais e seus discos.
Last video of Lecture 24. Formation of the Solar System (flashback); Spectral characteristics of flared disks. From dust to planets: overview. Growth of planet-size solid bodies. Formation of Planetesimals.
First video of Lecture 24. Formation of the Solar System (flashback); Spectral characteristics of flared disks. From dust to planets: overview. Growth of planet-size solid bodies. Formation of Planetesimals.
Last video of Lecture 23. Bipolar outflows. Observational evidence: jets in Herbig-Haro objects. Extremely High Velocity (EHV) gas; Standard High Velocity (classical component). Ionized High Velocity component. Neutral atomic (HI) and molecular (H2) component. EHV components and molecular bullets.
First video of Lecture 23. Bipolar outflows. Observational evidences: jets in Herbig-Haro objects. Extremely High Velocity (EHV) gas; Standard High Velocity (classical component). Ionized High Velocity component. Neutral atomic (HI) and molecular (H2) component. EHV components and molecular bullets.
Last video of Lecture 22. Historical background. Infrared and millimeter emission. Flat irradiated disks. Disk heating and structure: flared disks. Transitional disks. Proplyds
First video of Lecture 22. Historical background. Infrared and millimeter emission. Flat irradiated disks. Disk heating and structure: flared disks. Transitional disks. Proplyds
Last video of Lecture 21. Constructing the Luminosity Function: measuring distance from parallax; photometric (CMD) and spectroscopic (STMD) methods. Bias correction. The Mass-Magnitude relation; IMF parameters from Chabrier and Kroupa.
First video of Lecture 21. Constructing the Luminosity Function: measuring distance from parallax; photometric (CMD) and spectroscopic (STMD) methods. Bias correction. The Mass-Magnitude relation; IMF parameters from Chabrier and Kroupa.
Last video of Lecture 20. Introduction on how the star formation is distributed in space and time. Statistical techniques to describe spatial and kinematic distributions. The decline in number of stars clusters
First video of Lecture 20. Introduction on how the star formation is distributed in space and time. Statistical techniques to describe spatial and kinematic distributions. The decline in number of stars clusters.