Search Results - "Stutz, Amelia M."

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    Slingshot mechanism for clusters: Gas density regulates star density in the Orion Nebula Cluster (M42) by Stutz, Amelia M.

    “…Abstract We characterize the stellar and gas volume density, potential, and gravitational field profiles in the central ∼0.5 pc of the Orion Nebula Cluster…”
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    Gas velocity structure of the Orion A integral-shaped filament by González Lobos, Valentina, Stutz, Amelia M

    “…ABSTRACT We present analysis of the gas kinematics of the integral-shaped filament (ISF) in Orion A using four different molecular lines, 12CO (1−0), 13CO…”
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    300: An ACA 870 μm Continuum Survey of Orion Protostars and Their Evolution by Federman, Samuel, Megeath, S. Thomas, Tobin, John J., Sheehan, Patrick D., Pokhrel, Riwaj, Habel, Nolan, Stutz, Amelia M., Fischer, William J., Hartmann, Lee, Stanke, Thomas, Narang, Mayank, Osorio, Mayra, Atnagulov, Prabhani, Rahatgaonkar, Rohan

    Published in The Astrophysical journal (01-02-2023)
    “…Abstract We present an 870 μ m continuum survey of 300 protostars from the Herschel Orion Protostar Survey using the Atacama Compact Array (ACA). These data…”
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    The Herschel Orion Protostar Survey: Luminosity and Envelope Evolution by Fischer, William J., Megeath, S. Thomas, Furlan, Elise, Ali, Babar, Stutz, Amelia M., Tobin, John J., Osorio, Mayra, Stanke, Thomas, Manoj, P., Poteet, Charles A., Booker, Joseph J., Hartmann, Lee, Wilson, Thomas L., Myers, Philip C., Watson, Dan M.

    Published in The Astrophysical journal (10-05-2017)
    “…The Herschel Orion Protostar Survey obtained well-sampled 1.2-870 m spectral energy distributions (SEDs) of over 300 protostars in the Orion molecular clouds,…”
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    CHARACTERIZING THE YOUNGEST HERSCHEL-DETECTED PROTOSTARS. II. MOLECULAR OUTFLOWS FROM THE MILLIMETER AND THE FAR-INFRARED by Tobin, John J., Stutz, Amelia M., Manoj, P., Megeath, S. Thomas, Karska, Agata, Nagy, Zsofia, Wyrowski, Friedrich, Fischer, William J., Watson, Dan M., Stanke, Thomas

    Published in The Astrophysical journal (01-11-2016)
    “…ABSTRACT We present Combined Array for Research in Millimeter-wave Astronomy (CARMA) CO ( ) observations and Herschel PACS spectroscopy, characterizing the…”
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    Intensity-corrected Herschel Observations of Nearby Isolated Low-mass Clouds by Sadavoy, Sarah I., Keto, Eric, Bourke, Tyler L., Dunham, Michael M., Myers, Philip C., Stephens, Ian W., Di Francesco, James, Webb, Kristi, M. Stutz, Amelia, Launhardt, Ralf, J. Tobin, John

    Published in The Astrophysical journal (10-01-2018)
    “…Abstract We present intensity-corrected Herschel maps at 100, 160, 250, 350, and 500 μ m for 56 isolated low-mass clouds. We determine the zero-point…”
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    EVOLUTION OF MASS OUTFLOW IN PROTOSTARS by Watson, Dan M., Calvet, Nuria P., Fischer, William J., Forrest, W. J., Manoj, P., Megeath, S. Thomas, Melnick, Gary J., Najita, Joan, Neufeld, David A., Sheehan, Patrick D., Stutz, Amelia M., Tobin, John J.

    Published in The Astrophysical journal (01-09-2016)
    “…ABSTRACT We have surveyed 84 Class 0, Class I, and flat-spectrum protostars in mid-infrared [Si ii], [Fe ii], and [S i] line emission, and 11 of these in…”
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    Line profiles of cores within clusters – III. What is the most reliable tracer of core collapse in dense clusters? by Chira, Roxana-Adela, Smith, Rowan J., Klessen, Ralf S., Stutz, Amelia M., Shetty, Rahul

    “…Recent observational and theoretical investigations have emphasized the importance of filamentary networks within molecular clouds as sites of star formation…”
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    A High-mass, Young Star-forming Core Escaping from Its Parental Filament by Ren, Zhiyuan, Chen, Xi, Liu, Tie, Mannfors, Emma, Bronfman, Leonardo, Xu, Fengwei, Feng, Siyi, Liu, Hongli, Meng, Fanyi, Stutz, Amelia M., Li, Shanghuo, Lee, Chang Won, Wang, Ke, Zhou, Jianwen, Li, Di, Wang, Chen, Eswaraiah, Chakali, Tej, Anandmayee, Chen, Long-Fei, Shi, Hui

    Published in The Astrophysical journal (01-10-2023)
    “…Abstract We studied the unique kinematic properties in massive filament G352.63-1.07 at 10 3 au spatial scale with the dense molecular tracers observed with…”
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