Search Results - "Maud, Luke"
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Gas Density Perturbations Induced by One or More Forming Planets in the AS 209 Protoplanetary Disk as Seen with ALMA
Published in The Astrophysical journal (20-01-2019)“…The formation of planets occurs within protoplanetary disks surrounding young stars, resulting in perturbation of the gas and dust surface densities. Here we…”
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2
Salt-bearing Disk Candidates around High-mass Young Stellar Objects
Published in The Astrophysical journal (01-01-2023)“…Abstract Molecular lines tracing the orbital motion of gas in a well-defined disk are valuable tools for inferring both the properties of the disk and the star…”
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3
The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. II. A Statistical Characterization of Class 0 and Class I Protostellar Disks
Published in The Astrophysical journal (20-02-2020)“…We have conducted a survey of 328 protostars in the Orion molecular clouds with the Atacama Large Millimeter/submillimeter Array at 0.87 mm at a resolution of…”
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4
ALMA REVEALS THE ANATOMY OF THE mm-SIZED DUST AND MOLECULAR GAS IN THE HD 97048 DISK
Published in The Astrophysical journal (10-11-2016)“…ABSTRACT Transitional disks show a lack of excess emission at infrared wavelengths due to a large dust cavity, that is often corroborated by spatially resolved…”
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5
ALMA High-frequency Long-baseline Campaign in 2019: Band 9 and 10 In-band and Band-to-band Observations Using ALMA’s Longest Baselines
Published in The Astrophysical journal. Supplement series (01-08-2023)“…Abstract The Atacama Large Millimeter/submillimeter Array high-frequency long-baseline campaign in 2019 (HF-LBC-2019) was arranged to undertake band 9 (690…”
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Radiative transfer modelling of W33A MM1: 3D structure and dynamics of a complex massive star-forming region
Published in Monthly notices of the Royal Astronomical Society (01-08-2018)Get full text
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7
Evidence for the start of planet formation in a young circumstellar disk
Published in Nature astronomy (01-08-2018)“…The growth of dust grains in protoplanetary disks is a necessary first step towards planet formation 1 . This growth has been inferred from observations of…”
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8
The ALMA Interferometric Pipeline Heuristics
Published in Publications of the Astronomical Society of the Pacific (01-07-2023)“…Abstract We describe the calibration and imaging heuristics developed and deployed in the Atacama Large Millimeter/submillimeter Array (ALMA) interferometric…”
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9
Submillimeter array observations of NGC 2264-C: molecular outflows and driving sources
Published in Monthly notices of the Royal Astronomical Society (11-05-2016)“…We present 1.3 mm Submillimeter Array (SMA) observations at ∼3 arcsec resolution towards the brightest section of the intermediate/massive star-forming cluster…”
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10
ALMA High-frequency Long Baseline Campaign in 2021: Highest Angular Resolution Submillimeter Wave Images for the Carbon-rich Star R Lep
Published in The Astrophysical journal (01-11-2023)“…Abstract The Atacama Large Millimeter/submillimeter Array (ALMA) was used in 2021 to image the carbon-rich evolved star R Lep in Bands 8–10 (397–908 GHz) with…”
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11
ALMA High-frequency Long-baseline Campaign in 2017: An Investigation of Phase-referencing Cycle Times and Effective Baseline Lengths Using Band-to-band and In-band Phase Calibration Techniques
Published in The Astrophysical journal. Supplement series (01-03-2022)“…Abstract The Atacama Large Millimeter/submillimeter Array can achieve unprecedented spatial resolutions of 15 to 5 mas with the longest baselines of 16 km and…”
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12
Multiple chemical tracers finally unveil the intricate NGC 1333 IRAS 4A outflow system. FAUST XVI
Published in Monthly notices of the Royal Astronomical Society (29-05-2024)“…Abstract The exploration of outflows in protobinary systems presents a challenging yet crucial endeavour, offering valuable insights into the dynamic interplay…”
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13
ALMA Long Baseline Campaigns: Phase Characteristics of Atmosphere at Long Baselines in the Millimeter and Submillimeter Wavelengths
Published in Publications of the Astronomical Society of the Pacific (01-03-2017)“…We present millimeter- and submillimeter-wave phase characteristics measured between 2012 and 2014 of Atacama Large Millimeter/submillimeter Array long…”
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14
High angular resolution millimetre continuum observations and modelling of S140-IRS1
Published in Monthly notices of the Royal Astronomical Society (2013)“…We present high-resolution 1.3 mm continuum observations of the massive young stellar object S140-IRS1. S140-IRS1 is a disc wind prototype with elongated radio…”
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15
FAUST X: Formaldehyde in the Protobinary System [BHB2007] 11: Small Scale Deuteration
Published 01-09-2023“…A&A 678, A160 (2023) Context. Deuterium in H-bearing species is enhanced during the early stages of star formation, however, only a small number of high…”
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16
Infall and Outflow Motions towards a Sample of Massive Star Forming Regions from the RMS Survey
Published 09-03-2018“…We present the results of an outflow and infall survey towards a distance limited sample of 31 massive star forming regions drawn from the RMS survey. The…”
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17
Gas density perturbations induced by forming planet(s) in the AS 209 protoplanetary disk as seen with ALMA
Published 10-12-2018“…The formation of planets occurs within protoplanetary disks surrounding young stars, resulting in perturbation of the gas and dust surface densities. Here, we…”
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18
Missing water in Class I protostellar disks
Published 27-02-2020“…A&A 636, A26 (2020) Water is a key volatile that provides insights into the initial stages of planet formation. The low water abundances inferred from water…”
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19
The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. A Statistical Characterization of Class 0 and I Protostellar Disks
Published 13-01-2020“…We have conducted a survey of 328 protostars in the Orion molecular clouds with ALMA at 0.87 mm at a resolution of $\sim$0.1" (40 au), including observations…”
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Journal Article -
20
ALMA reveals the anatomy of the mm-sized dust and molecular gas in the HD 97048 disk
Published 10-11-2016“…2016, ApJ, 831, 200 Transitional disks show a lack of excess emission at infrared wavelengths due to a large dust cavity, that is often corroborated by…”
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