High-resolution Pan-STARRS and SMA observations of IRAS 23077+6707: A giant edge-on protoplanetary disk
arXiv:2402.01941 · doi:10.3847/2041-8213/ad3bb0
Abstract
We present resolved images of IRAS 23077+6707 ("Dracula's Chivito") in 1.3 mm/225 GHz thermal dust and CO gas emission with the Submillimeter Array (SMA) and optical (0.5-) scattered light with the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS). The Pan-STARRS data show a bipolar distribution of optically scattering dust that is characteristic for disks observed at high inclinations. Its scattered light emission spans , with two highly asymmetric filaments extending along the upper bounds of each nebula by . The SMA data measure 1.3 mm continuum dust as well as CO, CO and CO =21 line emission over - extents, with the gas presenting the typical morphology of a disk in Keplerian rotation, in both position-velocity space and in each CO line spectrum. IRAS 23077+6707 has no reported distance estimate, but if it is located in the Cepheus star-forming region (180-800 pc), it would have a radius spanning thousands of au. Taken together, we infer IRAS 23077+6707 to be a giant and gas-rich edge-on protoplanetary disk, which to our knowledge is the largest in extent so far discovered.
arXiv commentpublished in The Astrophysical Journal Letters 967:L2 (9pp), 2024 May 20
References in corpus (49)
- Array Programming with NumPy
- Astropy: A Community Python Package for Astronomy
- The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- Protoplanetary Disks and Their Evolution
- The Disk Substructures at High Angular Resolution Project (DSHARP): I. Motivation, Sample, Calibration, and Overview
- Interpreting Spectral Energy Distributions from Young Stellar Objects. I. A grid of 200,000 YSO model SEDs
- The Mass Dependence Between Protoplanetary Disks and their Stellar Hosts
- The Pan-STARRS1 Database and Data Products
- The Submillimeter Array
- ALMA Survey of Lupus Protoplanetary Disks I: Dust and Gas Masses
- Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region
- Observations of Protoplanetary Disk Structures
- ALMA Survey of Lupus Protoplanetary Disks II: Gas Disk Radii
- ALMA Observations of Circumstellar Disks in the Upper Scorpius OB Association
- HST/NICMOS Imaging of Disks and Envelopes Around Very Young Stars
- 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?
- Observations of edge-on protoplanetary disks with ALMA I. Results from continuum data
- The Circumstellar Disk of the Butterfly Star in Taurus
- On the Outer Edges of Protoplanetary Dust Disks
- Spectral Energy Distributions of Passive T Tauri Disks: Inclination
- A giant exoplanet orbiting a very low-mass star challenges planet formation models
- Signatures of broken protoplanetary discs in scattered light and in sub-millimetre observations
- Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Late infall causing disk misalignment and dynamic structures in SU Aur
- Study of the properties and spectral energy distributions of the Herbig AeBe stars HD 34282 and HD 141569
- Interaction between massive planets on inclined orbits and circumstellar discs
- High gas/dust size ratio indicating efficient radial drift in the mm-faint CX Tau disk
- Misaligned disks induced by infall
- An ALMA Continuum Survey of Circumstellar Disks in the Upper Scorpius OB Association
- Far-infrared to millimeter data of protoplanetary disks: dust growth in the Taurus, Ophiuchus, and Chamaeleon I star-forming regions
- Warping a protoplanetary disc with a planet on an inclined orbit
- The circumstellar disc in the Bok globule CB 26: Multi-wavelength observations and modelling of the dust disc and envelope
- Scattered light shadows in warped protoplanetary discs
- Pre-main sequence stars in the Cepheus flare region
- Protoplanetary Disks in the Orion Nebula Cluster: Gas Disk Morphologies and Kinematics as seen with ALMA
- Microwave Observations of Edge-on Protoplanetary Disks: Program Overview and First Results
- ALMA Survey of Lupus Class III Stars: Early Planetesimal Belt Formation and Rapid Disk Dispersal
- Circumbinary and circumstellar discs around the eccentric binary IRAS 04158+2805 -- a testbed for binary-disc interaction
- The Anatomy of an Unusual Edge-on Protoplanetary Disk. II. Gas temperature and a warm outer region
- The Anatomy of an Unusual Edge-on Protoplanetary Disk I. Dust Settling in a Cold Disk
- A Three Dimensional View of Gomez's Hamburger
- The surprising evolution of the shadow on the TW Hya disk
- Gomez's Hamburger (IRAS 18059-3211): A pre main-sequence A-type star
- Submillimeter Observations of the Young Low-Mass Object IRAS 04158+2805
- The view of the Cepheus flare
- Demographics of Protoplanetary Disks: A Simulated Population of Edge-on Systems
- An SMA Survey of Chemistry in Disks around Herbig AeBe Stars
- The physical conditions in Gomez's Hamburger (IRAS 18059-3211), a pre-MS rotating disk