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Szentgyorgyi Andrew - One of the best experts on this subject based on the ideXlab platform.

  • Dynamical Processes in the Planet-Forming Environment
    2019
    Co-Authors: Mcgehee Peregrine, Boss Alan, Close Laird, Dodson-robinson Sarah, Mawet Dimitri, Szentgyorgyi Andrew
    Abstract:

    The transfer of circumstellar disk mass and momentum onto the protostar and out into the environment occurs via a variety of mechanisms including magnetospheric accretion, jets, outflows, and disk winds. The interplay of these processes determine both the conditions under which planet formation occurs and the lifetime of the disk. Metallic emission lines, along with the Balmer series of Hydrogen, Probe the kinematics of gas within the planet-forming and central regions of circumstellar disks. High-spectral resolution study of these emission lines provides critical information on mass and momentum loss, turbulence, and disk wind origins

  • Astro2020 Science White Paper: Dynamical Processes in the Planet-Forming Environment
    2019
    Co-Authors: Mcgehee Peregrine, Boss Alan, Close Laird, Dodson-robinson Sarah, Mawet Dimitri, Szentgyorgyi Andrew
    Abstract:

    The transfer of circumstellar disk mass and momentum onto the protostar and out into the environment occurs via a variety of mechanisms including magnetospheric accretion, jets, outflows, and disk winds. The interplay of these processes determine both the conditions under which planet formation occurs and the lifetime of the disk. Metallic emission lines, along with the Balmer series of Hydrogen, Probe the kinematics of gas within the planet-forming and central regions of circumstellar disks. High-spectral resolution study of these emission lines provides critical information on mass and momentum loss, turbulence, and disk wind origins.Comment: Astro2020 Science White Pape

Mcgehee Peregrine - One of the best experts on this subject based on the ideXlab platform.

  • Dynamical Processes in the Planet-Forming Environment
    2019
    Co-Authors: Mcgehee Peregrine, Boss Alan, Close Laird, Dodson-robinson Sarah, Mawet Dimitri, Szentgyorgyi Andrew
    Abstract:

    The transfer of circumstellar disk mass and momentum onto the protostar and out into the environment occurs via a variety of mechanisms including magnetospheric accretion, jets, outflows, and disk winds. The interplay of these processes determine both the conditions under which planet formation occurs and the lifetime of the disk. Metallic emission lines, along with the Balmer series of Hydrogen, Probe the kinematics of gas within the planet-forming and central regions of circumstellar disks. High-spectral resolution study of these emission lines provides critical information on mass and momentum loss, turbulence, and disk wind origins

  • Astro2020 Science White Paper: Dynamical Processes in the Planet-Forming Environment
    2019
    Co-Authors: Mcgehee Peregrine, Boss Alan, Close Laird, Dodson-robinson Sarah, Mawet Dimitri, Szentgyorgyi Andrew
    Abstract:

    The transfer of circumstellar disk mass and momentum onto the protostar and out into the environment occurs via a variety of mechanisms including magnetospheric accretion, jets, outflows, and disk winds. The interplay of these processes determine both the conditions under which planet formation occurs and the lifetime of the disk. Metallic emission lines, along with the Balmer series of Hydrogen, Probe the kinematics of gas within the planet-forming and central regions of circumstellar disks. High-spectral resolution study of these emission lines provides critical information on mass and momentum loss, turbulence, and disk wind origins.Comment: Astro2020 Science White Pape

Boss Alan - One of the best experts on this subject based on the ideXlab platform.

  • Dynamical Processes in the Planet-Forming Environment
    2019
    Co-Authors: Mcgehee Peregrine, Boss Alan, Close Laird, Dodson-robinson Sarah, Mawet Dimitri, Szentgyorgyi Andrew
    Abstract:

    The transfer of circumstellar disk mass and momentum onto the protostar and out into the environment occurs via a variety of mechanisms including magnetospheric accretion, jets, outflows, and disk winds. The interplay of these processes determine both the conditions under which planet formation occurs and the lifetime of the disk. Metallic emission lines, along with the Balmer series of Hydrogen, Probe the kinematics of gas within the planet-forming and central regions of circumstellar disks. High-spectral resolution study of these emission lines provides critical information on mass and momentum loss, turbulence, and disk wind origins

  • Astro2020 Science White Paper: Dynamical Processes in the Planet-Forming Environment
    2019
    Co-Authors: Mcgehee Peregrine, Boss Alan, Close Laird, Dodson-robinson Sarah, Mawet Dimitri, Szentgyorgyi Andrew
    Abstract:

    The transfer of circumstellar disk mass and momentum onto the protostar and out into the environment occurs via a variety of mechanisms including magnetospheric accretion, jets, outflows, and disk winds. The interplay of these processes determine both the conditions under which planet formation occurs and the lifetime of the disk. Metallic emission lines, along with the Balmer series of Hydrogen, Probe the kinematics of gas within the planet-forming and central regions of circumstellar disks. High-spectral resolution study of these emission lines provides critical information on mass and momentum loss, turbulence, and disk wind origins.Comment: Astro2020 Science White Pape

Close Laird - One of the best experts on this subject based on the ideXlab platform.

  • Dynamical Processes in the Planet-Forming Environment
    2019
    Co-Authors: Mcgehee Peregrine, Boss Alan, Close Laird, Dodson-robinson Sarah, Mawet Dimitri, Szentgyorgyi Andrew
    Abstract:

    The transfer of circumstellar disk mass and momentum onto the protostar and out into the environment occurs via a variety of mechanisms including magnetospheric accretion, jets, outflows, and disk winds. The interplay of these processes determine both the conditions under which planet formation occurs and the lifetime of the disk. Metallic emission lines, along with the Balmer series of Hydrogen, Probe the kinematics of gas within the planet-forming and central regions of circumstellar disks. High-spectral resolution study of these emission lines provides critical information on mass and momentum loss, turbulence, and disk wind origins

  • Astro2020 Science White Paper: Dynamical Processes in the Planet-Forming Environment
    2019
    Co-Authors: Mcgehee Peregrine, Boss Alan, Close Laird, Dodson-robinson Sarah, Mawet Dimitri, Szentgyorgyi Andrew
    Abstract:

    The transfer of circumstellar disk mass and momentum onto the protostar and out into the environment occurs via a variety of mechanisms including magnetospheric accretion, jets, outflows, and disk winds. The interplay of these processes determine both the conditions under which planet formation occurs and the lifetime of the disk. Metallic emission lines, along with the Balmer series of Hydrogen, Probe the kinematics of gas within the planet-forming and central regions of circumstellar disks. High-spectral resolution study of these emission lines provides critical information on mass and momentum loss, turbulence, and disk wind origins.Comment: Astro2020 Science White Pape

Dodson-robinson Sarah - One of the best experts on this subject based on the ideXlab platform.

  • Dynamical Processes in the Planet-Forming Environment
    2019
    Co-Authors: Mcgehee Peregrine, Boss Alan, Close Laird, Dodson-robinson Sarah, Mawet Dimitri, Szentgyorgyi Andrew
    Abstract:

    The transfer of circumstellar disk mass and momentum onto the protostar and out into the environment occurs via a variety of mechanisms including magnetospheric accretion, jets, outflows, and disk winds. The interplay of these processes determine both the conditions under which planet formation occurs and the lifetime of the disk. Metallic emission lines, along with the Balmer series of Hydrogen, Probe the kinematics of gas within the planet-forming and central regions of circumstellar disks. High-spectral resolution study of these emission lines provides critical information on mass and momentum loss, turbulence, and disk wind origins

  • Astro2020 Science White Paper: Dynamical Processes in the Planet-Forming Environment
    2019
    Co-Authors: Mcgehee Peregrine, Boss Alan, Close Laird, Dodson-robinson Sarah, Mawet Dimitri, Szentgyorgyi Andrew
    Abstract:

    The transfer of circumstellar disk mass and momentum onto the protostar and out into the environment occurs via a variety of mechanisms including magnetospheric accretion, jets, outflows, and disk winds. The interplay of these processes determine both the conditions under which planet formation occurs and the lifetime of the disk. Metallic emission lines, along with the Balmer series of Hydrogen, Probe the kinematics of gas within the planet-forming and central regions of circumstellar disks. High-spectral resolution study of these emission lines provides critical information on mass and momentum loss, turbulence, and disk wind origins.Comment: Astro2020 Science White Pape

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