Search Results - "Stanke, Thomas"
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The Herschel Orion Protostar Survey: Luminosity and Envelope Evolution
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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The Evolution of Protostellar Outflow Cavities, Kinematics, and Angular Distribution of Momentum and Energy in Orion A: Evidence for Dynamical Cores
Published in The Astrophysical journal (01-04-2023)“…Abstract We present Atacama Large Millimeter/submillimeter Array observations of the ∼10,000 au environment surrounding 21 protostars in the Orion A molecular…”
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300: An ACA 870 μm Continuum Survey of Orion Protostars and Their Evolution
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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Confirmation of Enhanced Long-wavelength Dust Emission in OMC 2/3
Published in The Astrophysical journal (10-04-2020)“…Previous continuum observations from the MUSTANG camera on the Green Bank Telescope (GBT) of the nearby star-forming filament OMC 2/3 found elevated emission…”
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CHARACTERIZING THE YOUNGEST HERSCHEL-DETECTED PROTOSTARS. II. MOLECULAR OUTFLOWS FROM THE MILLIMETER AND THE FAR-INFRARED
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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Extension of HOPS out to 500 pc (eHOPS). I. Identification and Modeling of Protostars in the Aquila Molecular Clouds
Published in The Astrophysical journal. Supplement series (01-06-2023)“…Abstract We present a Spitzer/Herschel focused survey of the Aquila molecular clouds ( d ∼ 436 pc) as part of the eHOPS (extension of the Herschel orion…”
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Star Formation Under the Outflow: The Discovery of a Non-thermal Jet from OMC-2 FIR 3 and Its Relationship to the Deeply Embedded FIR 4 Protostar
Published in The Astrophysical journal (01-05-2017)“…We carried out multiwavelength (0.7-5 cm), multi-epoch (1994-2015) Very Large Array (VLA) observations toward the region enclosing the bright far-IR sources…”
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IPA: Class 0 Protostars Viewed in CO Emission Using JWST
Published in The Astrophysical journal (01-10-2024)“…Abstract We investigate the bright CO fundamental emission in the central regions of five protostars in their primary mass assembly phase using new…”
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JWST/MIRI Detection of Suprathermal OH Rotational Emissions: Probing the Dissociation of the Water by Lyα Photons near the Protostar HOPS 370
Published in Astrophysical journal. Letters (01-05-2024)“…Abstract Using the MIRI medium-resolution spectrometer on JWST, we have detected pure rotational, suprathermal OH emissions from the vicinity of the…”
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Evidence for large grains in the star-forming filament OMC 2/3
Published in Monthly notices of the Royal Astronomical Society (01-11-2014)Get full text
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Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy
Published in Open research Europe (2024)“…As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop a greater understanding for the complex relationships between the…”
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MULTIWAVELENGTH OBSERVATIONS OF V2775 Ori, AN OUTBURSTING PROTOSTAR IN L 1641: EXPLORING THE EDGE OF THE FU ORIONIS REGIME
Published in The Astrophysical journal (01-09-2012)Get full text
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A HERSCHEL AND APEX CENSUS OF THE REDDEST SOURCES IN ORION: SEARCHING FOR THE YOUNGEST PROTOSTARS
Published in The Astrophysical journal (10-04-2013)“…We perform a census of the reddest, and potentially youngest, protostars in the Orion molecular clouds using data obtained with the PACS instrument on board…”
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Evidence for large grains in the star-forming filament OMC 2/3
Published in Monthly notices of the Royal Astronomical Society (01-11-2014)“…We present a new 3.3 mm continuum map of the Orion Molecular Cloud (OMC) 2/3 region. When paired with previously published maps of 1.2 mm continuum and…”
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The Rate, Amplitude, and Duration of Outbursts from Class 0 Protostars in Orion
Published in Astrophysical journal. Letters (01-01-2022)“…Abstract At least half of a protostar’s mass is accreted in the Class 0 phase, when the central protostar is deeply embedded in a dense, infalling envelope. We…”
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The Herschel Orion Protostar Survey: Far-infrared Photometry and Colors of Protostars and Their Variations across Orion A and B
Published in The Astrophysical journal (01-12-2020)“…Abstract The degree to which the properties of protostars are affected by environment remains an open question. To investigate this, we look at the Orion A and…”
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A Study of 90 GHz Dust Emissivity on Molecular Cloud and Filament Scales
Published in The Astrophysical journal (01-04-2022)“…Abstract Recent observations from the MUSTANG2 instrument on the Green Bank Telescope have revealed evidence of enhanced long-wavelength emission in the dust…”
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Investigating Protostellar Accretion-driven Outflows across the Mass Spectrum: JWST NIRSpec Integral Field Unit 3–5 μm Spectral Mapping of Five Young Protostars
Published in The Astrophysical journal (01-05-2024)“…Abstract Investigating Protostellar Accretion is a Cycle 1 JWST program using the NIRSpec+MIRI integral field units to obtain 2.9–28 μ m spectral cubes of five…”
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CHARACTERIZING THE YOUNGEST HERSCHEL -DETECTED PROTOSTARS. I. ENVELOPE STRUCTURE REVEALED BY CARMA DUST CONTINUUM OBSERVATIONS
Published in The Astrophysical journal (10-01-2015)“…We present Combined Array for Research in Millimeter-wave Astronomy 2.9mm dust continuum emission observations of a sample of 14 Herschel-detected Class 0…”
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