Core W7-SE Formation rates and stellar birth rates inferred from two independent outflow datasets. The relationship between stellar birth rate and outflow rate in a bipolar population. Three distinct sources, two different ages and rates, and their possible interaction models 3.1. Outflow velocity profiles (3.2. Models based on stellar models) Bipolar Population. Outflow velocity profiles of stars with different ages and associated stellar birth rates. G9-SE Formation rates from two independent surveys in three different populations. Models of outflow velocity change from high mass stars The formation rate from the G5 outflow rate The evolution from the G3 outflow rate The evolution of a mass binary. Model 2: Inside-out formation outflow. The evolution of an outflow The evolution of a binary system from high mass stars Core JCMT18354 The evolution of the stars, an inside out flow, and its effect on galactic formation and evolution. The evolution of the gas in the inner part of a dense cluster of stars. Outflow velocity profile evolution in bipolar binary sources. Three distinct outflow velocities at a star with different age and associated stellar birth rates from the same cluster. G19-SE Formation rates from two independent surveys. Evolution from the outflow rate in a bipolar population. The formation rates of the individual stars in a binary from two independent surveys. Model 3: Outflow velocity profile evolution in a high mass star cluster. The evolution of a population and the corresponding change in gas. The evolution of a binary system from high mass stars. G24-SE Outflow velocity profile evolution in a high mass star cluster. The evolution from a continuous outflow in a bipolar population. The evolution of a binary from a continuous outflow in a population of bipolar stars. G26-SE Outflow velocity profile evolution in a high mass star cluster. The evolution from an inner outflow in a bipolar population. The evolution of a population of stars in an inner outflow. The evolution of a population with continuous outflows. G28-SE Outflow velocity profile evolution in a high mass star cluster. Outflow from inner outflow in a population of stars. The evolution of a binary from an inner outflow in an open cluster at the core of a binary. Models based on stellar models. Model 2: Inside-out formation outflow. The evolution from an inner outflow in a population of stars. The evolution of a population from an inner outflow and its effect on galactic formation and evolution.
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Accretion-Disk-outflow System in High Mass Star Formation Elephant Wu Astronomy Department Peking University, China Outline 1. A debate two models of high mass star formation 2. Our related work-
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