| Description |
We propose to utilize the unprecedented spatial resolution and sensitivity of
Herschel at far-infrared and submm wavelengths to observe nearly all known FU Orionis objects, the dramatic result of burst accretion events in protostellar disks. The known FUors represent a vital window into a key process of star
formation rather than a rare and peculiar event in the lives of a few stars. In addition, FUors provide a natural laboratory that probes the effect on enhanced heating on disk composition and structure.
Our objectives are to (1) Study the structure of known envelopes and constrain the amount of remnant envelope material around the remainder; (2) characterize the physical and chemical properties of the disks and envelope, the parameters that set the initial conditions for planet formation in T Tauri disks;
(3) observe solid-state, atomic, and molecular spectral features toward FUors
in order to determine the effects of increased luminosity on mineralogy, disk
chemistry, and envelope material. In order to do this we will use all three instruments onboard Herschel, providing a comprehensive survey of FUors. |
| Publication |
An Analysis of the Environments of FU Orionis Objects with Herschel . Green Joel D. et al. . The Astrophysical Journal, Volume 772, Issue 2, article id. 117, 23 pp. (2013). . 772 . 10.1088\/0004-637X\/772\/2\/117 . 2013ApJ...772..117G ,
A Multi-epoch, Multiwavelength Study of the Classical FUor V1515 Cyg Approaching Quiescence . Szabó Zs. M. et al. . The Astrophysical Journal . null . null . 2022ApJ...936...64S ,
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