Spitzer-IRS Observations of FU Orionis Objects
arXiv:astro-ph/0605365 · doi:10.1086/505932
Abstract
We present 5-35 m spectra, taken with the Infrared Spectrograph (IRS) on the Spitzer Space Telescope, of five FU Orionis objects: FU Ori, V1515 Cyg, V1057 Cyg, BBW 76, and V346 Nor. All but V346 Nor reveal amorphous silicate grains in emission at 10 m and 20 m, and show water-vapor absorption bands at 5.8 and 6.8 m and SiO or possibly methane absorption at 8 m. These absorption features closely match these bands in model stellar photospheres -- signs of the gaseous photospheres of the inner regions of these objects' accretion disks. The continuum emission at 5-8 m is also consistent with such disks, and, for FU Orionis and BBW 76, longer-wavelength emission may be fit by a model which includes moderate disk flaring. V1057 Cyg and V1515 Cyg have much more emission at longer wavelengths than the others, perhaps evidence of substantial remnant of their natal, infalling envelopes.
30 pages, 8 figures, accepted by ApJ
References in corpus (16)
- The Spitzer Space Telescope Mission
- Interstellar Dust Grains
- Spectral Energy Distributions of T Tauri Stars With Passive Circumstellar Disks
- The Infrared Spectrograph on the Spitzer Space Telescope
- Using FU Orionis Outbursts to Constrain Self-Regulated Protostellar Disk Models
- Accretion Disks Around Young Objects. II. Tests of Well-Mixed Models with Ism Dust
- The SMART Data Analysis Package for the Infrared Spectrograph on the Spitzer Space Telescope
- Unveiling the Inner Disk Structure of T Tauri Stars
- Spectral Irradiance Calibration in the Infrared. XIII. "Supertemplates" and On-Orbit Calibrators for SIRTF's Infrared Array Camera (IRAC)
- Bipolar molecular outflows driven by hydromagnetic protostellar winds
- Spherically symmetric model atmospheres for low mass pre-Main Sequence stars with effective temperatures between 2000 and 6800 K
- Dust Processing in Disks around T Tauri Stars
- The photometric evolution of FU Orionis objects: disc instability and wind-envelope interaction
- New insights on the AU-scale circumstellar structure of FU Orionis
- A Comprehensive Study of the L1551 IRS 5 Binary System
- Keck Interferometer Observations of FU Orionis Objects
Cited by in corpus (57)
- Interpreting Spectral Energy Distributions from Young Stellar Objects. I. A grid of 200,000 YSO model SEDs
- The formation and evolution of planetary systems: Grain growth and chemical processing of dust in T Tauri systems
- The Hot Inner Disk of FU Ori
- A New Look at T Tauri Star Forbidden Lines: MHD Driven Winds from the Inner Disk
- Spitzer IRS Spectra and Envelope Models of Class I Protostars in Taurus
- Gravitational Instabilities, Chondrule Formation, and the FU Orionis Phenomenon
- Evolution of dust and ice features around FU Orionis objects
- Silicate Dust in Evolved Protoplanetary Disks: Growth, Sedimentation, and Accretion
- EX Lupi in quiescence
- Relation between the luminosity of young stellar objects and their circumstellar environment
- Near-Infrared High-Resolution Imaging Polarimetry of FU Ori-Type Objects: Towards A Unified Scheme for Low-Mass Protostellar Evolution
- Long-wavelength excesses of FU Orionis objects: flared outer disks or infalling envelopes?
- A Spitzer-IRS Detection of Crystalline Silicates in a Protostellar Envelope
- High Resolution Near-Infrared Spectroscopy of FUors and FUor-like stars
- Optical and infrared properties of V1647 Orionis during the 2003-2006 outburst. II. Temporal evolution of the eruptive source
- An Analysis of the Environments of FU Orionis Objects with Herschel
- V1647 Orionis: One Year into Quiescence
- Dust Transport and Processing in Centrifugally Driven Protoplanetary Disk Winds
- Massive compact disks around FU Orionis-type young eruptive stars revealed by ALMA
- Distinguishing between different mechanisms of FU-Orionis-type luminosity outbursts
- A 1.3 mm SMA Survey of 29 Variable Young Stellar Objects
- Millimeter-sized Dust Grains Appear Surviving the Water-sublimating Temperature in the Inner 10 au of the FU Ori Disk
- Diagnosing 0.1-10 au scale morphology of the FU\,Ori disk using ALMA and VLTI/GRAVITY
- Disentangling the Environment of the FU Orionis Candidate HBC 722 with Herschel
- V346 Normae: First post-outburst observations of an FU Orionis star
- Resolving the Sub-AU-Scale Gas and Dust Distribution in FU Orionis Sources
- Mass transport from the envelope to the disk of V346 Nor: a case study for the luminosity problem in an FUor-type young eruptive star
- The progenitor of the FUor-type young eruptive star 2MASS J06593158-0405277
- X-ray Emission from the FU Orionis Star V1735 Cygni
- Interferometric view of the circumstellar envelopes of northern FU Orionis-type stars
- Variability at the Edge: Optical Near/IR Rapid Cadence Monitoring of Newly Outbursting FU Orionis Object HBC 722
- High-resolution polarimetry of Parsamian 21: revealing the structure of an edge-on FU Ori disc
- FU Orionis outbursts, preferential recondensation of water ice, and the formation of giant planets
- A multi-epoch, multi-wavelength study of the classical FUor V1515 Cyg approaching quiescence
- HD 145263: Spectral Observations of Silica Debris Disk Formation via Extreme Space Weathering?
- The disk of FU Orionis viewed with MATISSE/VLTI: first interferometric observations in and bands
- Cold CO gas in the envelopes of FU Orionis-type young eruptive stars
- Millimeter interferometric observations of FU Orionis-type objects in Cygnus
- Chandra Reveals Variable Multi-Component X-ray Emission from FU Orionis
- An ALMA Study of the FU-Ori Type Object V900 Mon: Implications for the Progenitor
- Mid-IR observations of circumstellar disks -- Part III: A mixed sample of PMS stars and Vega-type objects
- Emission from Water Vapor and Absorption from Other Gases at 5-7.5 Microns in Spitzer-IRS Spectra of Protoplanetary Disks
- The Mid-Infrared Evolution of the FU Orionis Disk
- Testing the Binary Trigger Hypothesis in FUors
- An APEX study of molecular outflows in FUor-type stars
- Grain growth in newly discovered young eruptive stars
- APEX Observations of the CO Envelope around the Young FUor-type Star V883 Ori
- Accretion Burst Crystallizes Silicates in a Planet-Forming Disk
- Disc light variability in the FUor star V646 Puppis as observed by TESS and from the ground
- Time-domain study of the young massive cluster Westerlund 2 with the Hubble Space Telescope. I
- Time-dependent response of protoplanetary disk temperature to an FU Ori-type luminosity outburst
- Molecular inventory of a young eruptive star's environment -- Case study of the classical FU Orionis star V1057 Cyg
- Infrared and sub-mm observations of outbursting young stars with Herschel and Spitzer
- Spectro-astrometry of V1515 Cyg
- A study of the photometric and spectroscopic variations of the prototypical FU Orionis-type star V1057 Cyg
- Simulation of a protoplanetary disk accretion activity due to a collision with a gas stream
- Episodic accretion in focus: revealing the environment of FU Orionis-type stars