An ALMA survey of $\lambda$ Orionis disks: from supernovae to planet formation

Abstract

Protoplanetary disk surveys by the Atacama Large Millimeter/sub-millimeter Array (ALMA) are now probing a range of environmental conditions, from low-mass star-forming regions like Lupus to massive OB clusters like $\sigma$ Orionis. Here we conduct an ALMA survey of protoplanetary disks in $\lambda$ Orionis, a ~5 Myr old OB cluster in Orion, with dust mass sensitivities comparable to the surveys of nearby regions (~0.4 $M_{\oplus }$). We assess how massive OB stars impact planet formation, in particular from the supernova that may have occurred ~1 Myr ago in the core of $\lambda$ Orionis; studying these effects is important as most planetary systems, including our Solar System, are likely born in cluster environments. We find that the effects of massive stars, in the form of pre-supernova feedback and/or a supernova itself, do not appear to significantly reduce the available planet-forming material otherwise expected at the evolved age of $\lambda$ Orionis. We also compare a lingering massive "outlier" disk in $\lambda$ Orionis to similar systems in other evolved regions, hypothesizing that these outliers host companions in their inner disks that suppress disk dispersal to extend the lifetimes of their outer primordial disks. We conclude with numerous avenues for future work, highlighting how $\lambda$ Orionis still has much to teach us about perhaps one of the most common types of planet-forming environments in the Galaxy.

arXiv comment21 pages, 8 figures, 3 tables. Accepted to AAS Journals

References in corpus (102)

• Astropy: A Community Python Package for Astronomy
• Gaia Data Release 2. Summary of the contents and survey properties
• The Gaia mission
• Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
• The Infrared Array Camera (IRAC) for the Spitzer Space Telescope
• The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
• Estimating distances from parallaxes IV: Distances to 1.33 billion stars in Gaia Data Release 2
• New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit
• The Disk Substructures at High Angular Resolution Project (DSHARP): I. Motivation, Sample, Calibration, and Overview
• The Keck Planet Search: Detectability and the Minimum Mass and Orbital Period Distribution of Extrasolar Planets
• The Occurrence and Architecture of Exoplanetary Systems
• Circumstellar Dust Disks in Taurus-Auriga: The Submillimeter Perspective
• The Mass Dependence Between Protoplanetary Disks and their Stellar Hosts
• ALMA Survey of Lupus Protoplanetary Disks I: Dust and Gas Masses
• Ringed Substructure and a Gap at 1 AU in the Nearest Protoplanetary Disk
• The Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics From 10-100 AU
• The Birth Environment of the Solar System
• A Steeper than Linear Disk Mass-Stellar Mass Scaling Relation
• ALMA Survey of Lupus Protoplanetary Disks II: Gas Disk Radii
• Imaging Extrasolar Giant Planets
• On the origin of the O and B-type stars with high velocities II Runaway stars and pulsars ejected from the nearby young stellar groups
• An ALMA Survey of Protoplanetary Disks in the $\sigma$ Orionis Cluster
• The APOGEE-2 Survey of the Orion Star Forming Complex II: Six-dimensional structure
• ALMA Observations of Circumstellar Disks in the Upper Scorpius OB Association
• Protoplanetary disk lifetimes vs stellar mass and possible implications for giant planet populations
• Transitional and Pre-Transitional disks: Gap Opening by Multiple Planets?
• Before the first supernova: combined effects of HII regions and winds on molecular clouds
• Pre-main-sequence isochrones -- II. Revising star and planet formation timescales
• The Ophiuchus DIsc Survey Employing ALMA (ODISEA) - I : project description and continuum images at 28 au resolution
• Why do protoplanetary disks appear not massive enough to form the known exoplanet population?
• Destruction of protoplanetary disks in the Orion Nebula Cluster
• A Millimeter Continuum Size-Luminosity Relationship for Protoplanetary Disks
• One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering
• Lupus disks with faint CO isotopologues: low gas/dust or large carbon depletion?
• Spitzer observations of the Orion OB1 association: disk census in the low mass stars
• The Photoevaporation of Discs Around Young Stars in Massive Clusters
• Setting the volatile composition of (exo)planet-building material. Does chemical evolution in disk midplanes matter?
• Protoplanetary disc truncation mechanisms in stellar clusters: comparing external photoevaporation and tidal encounters
• The origin of runaway stars
• A Keck High Resolution Spectroscopic Study of the Orion Nebula Proplyds
• Evolution of Giant Planets in Eccentric Disks
• Scaling Relations Associated with Millimeter Continuum Sizes in Protoplanetary Disks
• Physical properties of dusty protoplanetary disks in Lupus: evidence for viscous evolution?
• The Disk Substructures at High Angular Resolution Project (DSHARP): IV. Characterizing substructures and interactions in disks around multiple star systems
• External photoevaporation of protoplanetary discs in sparse stellar groups: the impact of dust growth
• ALMA Observations of the Orion Proplyds
• CO destruction in protoplanetary disk midplanes: inside versus outside the CO snow surface
• New insights into the nature of transition disks from a complete disk survey of the Lupus star forming region
• Empirical Isochrones for Low Mass Stars in Nearby Young Associations
• Fingerprints of giant planets in the photospheres of Herbig stars
• Unlocking CO Depletion in Protoplanetary Disks I. The Warm Molecular Layer
• Refining the Census of the Upper Scorpius Association with Gaia
• The Mass Budget of Planet Forming Discs: Isolating the Epoch of Planetesimal Formation
• The many-faceted light curves of young disk-bearing stars in Upper Sco and $\rho$ Oph observed by $K2$ Campaign 2
• Chemical abundances of magnetic and non-magnetic Herbig Ae/Be stars
• Spectroscopy of Very Low Mass Stars and Brown Dwarfs in the Lambda Orionis Star Forming Region. I. Enlarging the census down to the planetary mass domain in Collinder 69
• Chasing Shadows: Rotation of the Azimuthal Asymmetry in the TW Hya Disk
• The Disk Substructures at High Angular Resolution Project (DSHARP): X. Multiple rings, a misaligned inner disk, and a bright arc in the disk around the T Tauri star HD 143006
• Bright C2H emission in protoplanetary disks in Lupus: high volatile C/O>1 ratios
• Star formation and disk properties in Pismis 24
• Exclusion of Cosmic Rays in Protoplanetary Disks. II. Chemical Gradients and Observational Signatures
• ALMA survey of Class II protoplanetary disks in Corona Australis: a young region with low disk masses
• Kinematics of the CO Gas in the Inner Regions of the TW Hya Disk
• The evolution of dust in discs influenced by external photoevaporation
• Physical conditions in the central molecular zone inferred by H3+
• FLAMES spectroscopy of low-mass stars in the young clusters sigma Ori and lambda Ori
• Investigating the Cosmic-Ray Ionization Rate Near the Supernova Remnant IC 443 Through H3+ Observations
• Observations of Solids in Protoplanetary Disks
• External photoevaporation of circumstellar disks constrains the timescale for planet formation
• Proplyds around a B1 star - 42 Orionis in NGC 1977
• First evidence of external disc photoevaporation in a low mass star forming region: the case of IM Lup
• Have proto-planetary discs formed planets?
• The dispersal of protoplanetary disks around binary stars
• Variable Outer Disk Shadowing Around the Dipper Star RX J1604.3-2130
• 870 micron Imaging of a Transitional Disk in Upper Scorpius: Holdover from the Era of Giant Planet Formation?
• Are Inner Disc Misalignments Common? ALMA Reveals an Isotropic Outer Disc Inclination Distribution for Young Dipper Stars
• Hints on the origins of particle traps in protoplanetary disks given by the $M_{\mathrm{dust}}-M_{\star }$ relation
• A survey for low mass spectroscopic binary stars in the young clusters around sigma Orionis and lambda Orionis
• Corona-Australis DANCe. I. Revisiting the census of stars with Gaia-DR2 data
• Prevalent externally-driven protoplanetary disc dispersal as a function of the galactic environment
• Supernova feedback and the energy deposition in molecular clouds
• A high-resolution spectropolarimetric survey of Herbig Ae/Be stars - II. Rotation
• Spitzer Observations of the Lambda Orionis cluster. II. Disks around solar-type and low mass stars
• Where can a Trappist-1 planetary system be produced?
• 13C17O suggests gravitational instability in the HL Tau disc
• Disk masses in the Orion Molecular Cloud-2: distinguishing time and environment
• Save the Planet, Feed the Star: How Super-Earths Survive Migration and Drive Disk Accretion
• Spitzer Observations of the Lambda Orionis cluster I: the frequency of young debris disks at 5 Myr
• PDS 70: A transition disk sculpted by a single planet
• Photochemical-dynamical models of externally FUV irradiated protoplanetary discs
• The ALMA Lupus protoplanetary disk survey: evidence for compact gas disks and molecular rings from CN
• Surface Geometry of Protoplanetary Disks Inferred From Near-Infrared Imaging Polarimetry
• How Consumption and Repulsion Set Planetary Gap Depths and the Final Masses of Gas Giants
• Constraining the radial drift of millimeter-sized grains in the protoplanetary disks in Lupus
• Flipping-up the field: gravitational feedback as a mechanism for young clusters dispersal
• Gaia DR2 view of the Lupus V-VI clouds: the candidate diskless young stellar objects are mainly background contaminants
• External photoevaporation of protoplanetary discs in Cygnus OB2: linking discs to star formation dynamical history
• Probing the presence of planets in transition discs' cavities via warps: the case of TW Hya
• Discovery of an old photoevaporating disk in sigma Orionis
• The Observational Anatomy of Externally Photoevaporating Planet-Forming Discs I: Atomic Carbon
• Astronomical Evidence for the Rapid Growth of Millimeter Sized Particles in Protoplanetary Disks
• Hydrodynamic ablation of protoplanetary disks via supernovae

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• A stellar mass dependence of structured disks: a possible link with exoplanet demographics
• Bridging the gap between protoplanetary and debris disks: separate evolution of millimeter and micrometer-sized dust
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• The influence of the environment on the spin evolution of low-mass stars. I. External photoevaporation of circumstellar disks
• The impact of dynamic pressure bumps on the observational properties of protoplanetary disks
• Determining Dust Properties in Protoplanetary Disks: SED-derived Masses and Settling With ALMA
• Warm millimetre dust in protoplanetary discs near massive stars
• Probing protoplanetary disk evolution in the Chamaeleon II region
• Evolution of circumstellar discs in young star-forming regions
• Chemical modeling of Orion Nebula Cluster disks: evidence for massive, compact gas disks with ISM-like gas-to-dust ratios
• A Novel Method to Estimate the FUV Flux and a Catalogue for Star-Hosting Discs in Nearby Star-Forming Regions
• The statistical properties of protostellar discs and their dependence on metallicity
• Linking ice and gas in the Lambda Orionis Barnard 35A cloud
• A study of the frequency and characteristics of stellar companions and Jupiter-like planets in nearby open clusters
• The evolution of protoplanetary disc radii and disc masses in star-forming regions
• A complete Herbig disk mass survey in Orion
• A SPHERE survey of self-shadowed planet-forming disks
• Gaps and Rings: A Near-Universal Trait of Extended Protoplanetary Discs
• The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars VI. Insights from Radiative Transfer Modeling
• The Sejong Open Cluster Survey (SOS). VII. A Photometric Study of the Young Open Cluster IC 1590