Search Results - "Manara, C. F."
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A STEEPER THAN LINEAR DISK MASS-STELLAR MASS SCALING RELATION
Published in The Astrophysical journal (10-11-2016)“…ABSTRACT The disk mass is among the most important input parameter for every planet formation model to determine the number and masses of the planets that can…”
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ALMA Survey of Lupus Protoplanetary Disks. II. Gas Disk Radii
Published in The Astrophysical journal (20-05-2018)“…We present Atacama Large Millimeter/Sub-Millimeter Array (ALMA) Band 6 observations of a complete sample of protoplanetary disks in the young (∼1-3 Myr) Lupus…”
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ALMA SURVEY OF LUPUS PROTOPLANETARY DISKS. I. DUST AND GAS MASSES
Published in The Astrophysical journal (01-09-2016)“…ABSTRACT We present the first high-resolution sub-millimeter survey of both dust and gas for a large population of protoplanetary disks. Characterizing…”
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The little dippers: transits of star-grazing exocomets?
Published in Monthly notices of the Royal Astronomical Society (01-03-2019)Get full text
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Multiwavelength continuum sizes of protoplanetary discs: scaling relations and implications for grain growth and radial drift
Published in Monthly notices of the Royal Astronomical Society (01-09-2021)“…ABSTRACT We analyse spatially resolved ALMA observations at 0.9, 1.3, and 3.1 mm for the 26 brightest protoplanetary discs in the Lupus star-forming region. We…”
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Variable Outer Disk Shadowing around the Dipper Star RXJ1604.3–2130
Published in The Astrophysical journal (01-12-2018)“…Abstract Low brightness dips have recently been observed in images of protoplanetary disks, and they are believed to be shadows by the inner disk. We present…”
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Homogeneous Analysis of the Dust Morphology of Transition Disks Observed with ALMA: Investigating Dust Trapping and the Origin of the Cavities
Published in The Astrophysical journal (20-05-2018)“…We analyze the dust morphology of 29 transition disks (TDs) observed with Atacama Large (sub-)Millimeter Array (ALMA) at (sub-)millimeter emission. We perform…”
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The Young Suns Exoplanet Survey: Detection of a wide-orbit planetary-mass companion to a solar-type Sco-Cen member
Published in Monthly notices of the Royal Astronomical Society (01-02-2020)“…ABSTRACT The Young Suns Exoplanet Survey consists of a homogeneous sample of 70 young, solar-mass stars located in the Lower Centaurus-Crux subgroup of the…”
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The first ALMA survey of protoplanetary discs at 3 mm: demographics of grain growth in the Lupus region
Published in Monthly notices of the Royal Astronomical Society (10-08-2021)“…ABSTRACT We present the first ALMA survey of protoplanetary discs at 3 mm, targeting 36 young stellar objects in the Lupus star-forming region with deep…”
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HUBBLE SPACE TELESCOPE MEASURES OF MASS ACCRETION RATES IN THE ORION NEBULA CLUSTER
Published in The Astrophysical journal (20-08-2012)“…The present observational understanding of the evolution of the mass accretion rates (M sub(acc)) in pre-main-sequence stars is limited by the lack of accurate…”
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ALMA survey of Lupus class III stars: Early planetesimal belt formation and rapid disc dispersal
Published in Monthly notices of the Royal Astronomical Society (01-02-2021)“…ABSTRACT Class III stars are those in star forming regions without large non-photospheric infrared emission, suggesting recent dispersal of their…”
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Localized thermonuclear bursts from accreting magnetic white dwarfs
Published in Nature (London) (21-04-2022)“…Nova explosions are caused by global thermonuclear runaways triggered in the surface layers of accreting white dwarfs 1 – 3 . It has been predicted 4 – 6 that…”
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The Ṁ–M relation of pre-main-sequence stars: a consequence of X-ray driven disc evolution
Published in Monthly notices of the Royal Astronomical Society (21-03-2014)“…We analyse current measurements of accretion rates on to pre-main-sequence stars as a function of stellar mass, and conclude that the steep dependence of…”
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The ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109
Published in The Astronomical journal (01-03-2022)“…Abstract The Hubble UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Director’s Discretionary Program of low-mass pre-main-sequence stars,…”
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North-PHASE: studying periodicity, hot spots, accretion stability, and early evolution in young stars in the Northern hemisphere
Published in Monthly notices of the Royal Astronomical Society (01-08-2024)“…ABSTRACT We present the overview and first results from the North-PHASE Legacy Survey, which follows six young clusters for five years, using the 2 deg$^2$ FoV…”
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A UV-TO-MIR MONITORING OF DR TAU: EXPLORING HOW WATER VAPOR IN THE PLANET FORMATION REGION IS AFFECTED BY STELLAR ACCRETION VARIABILITY
Published in The Astrophysical journal (01-01-2014)“…Young stars are known to show variability due to non-steady mass accretion rate from their circumstellar disks. Accretion flares can produce strong energetic…”
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The peculiar dipping events in the disc-bearing young-stellar object EPIC 204278916
Published in Monthly notices of the Royal Astronomical Society (01-12-2016)“…EPIC 204278916 has been serendipitously discovered from its K2 light curve that displays irregular dimmings of up to 65 per cent for ...25 consecutive days out…”
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Rapid CO gas dispersal from NO Lup’s class III circumstellar disc
Published in Monthly notices of the Royal Astronomical Society. Letters (01-03-2021)“…ABSTRACT We observed the K7 class III star NO Lup in an ALMA survey of the 1–3 Myr Lupus association and detected circumstellar dust and CO gas. Here we show…”
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Strong biases in estimating the time dependence of mass accretion rates in young stars
Published in Monthly notices of the Royal Astronomical Society (21-04-2014)“…The temporal decay of mass accretion in young stars is a fundamental tracer of the early evolution of circumstellar discs. Through population syntheses, we…”
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The 2015-2016 Outburst of the Classical EXor V1118 Ori
Published in The Astrophysical journal (20-04-2017)“…After a quiescence period of about 10 years, the classical EXor source V1118 Ori has undergone an accretion outburst in 2015 September. The maximum brightness…”
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