2-D Radiative Transfer in Protostellar Envelopes: I. Effects of Geometry on Class I Sources
arXiv:astro-ph/0303479 · doi:10.1086/375415
Abstract
We present 2-D radiation transfer models of Class I Protostars and show the effect of including more realistic geometries on the resulting spectral energy distributions and images. We begin with a rotationally flattened infalling envelope as our comparison model, and add a flared disk and bipolar cavity. The disk affects the spectral energy distribution most strongly at edge-on inclinations, causing a broad dip at about 10 um (independent of the silicate feature) due to high extinction and low scattering albedo in this wavelength region. The bipolar cavities allow more direct stellar+disk radiation to emerge into polar directions, and more scattering radiation to emerge into all directions. The wavelength-integrated flux, often interpreted as luminosity, varies with viewing angle, with pole-on viewing angles seeing 2-4 times as much flux as edge-on, depending on geometry. Thus, observational estimates of luminosity should take into account the inclination of a source. The envelopes with cavities are significantly bluer in near-IR and mid-IR color-color plots than those without cavities. Using 1-D models to interpret Class I sources with bipolar cavities would lead to an underestimate of envelope mass and an overestimate of the implied evolutionary state. We compute images at near-, mid-, and far-IR wavelengths. We find that the mid-IR colors and images are sensitive to scattering albedo, and that the flared disk shadows the midplane on large size scales at all wavelengths plotted. Finally, our models produce polarization spectra which can be used to diagnose dust properties, such as albedo variations due to grain growth. Our results of polarization across the 3.1 um ice feature agree well with observations for ice mantles covering 5% of the radius of the grains.
Accepted for publication in ApJ, 37 pages, 13 figures (several figures reduced in quality; find original version at http://gemelli.colorado.edu/~bwhitney/preprints.html)
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- A 1000 AU Scale Molecular Outflow Driven by a Protostar with an age of <4000 Years
- SABOCA 350-micron and LABOCA 870-micron dust continuum imaging of IRAS 05399-0121: mapping the dust properties of a pre- and protostellar core system
- Infrared Excess of a Large OB Star Sample
- A Parsec-scale Bipolar H Outflow in the Massive Star Forming Infrared Dark Cloud Core MSXDC G053.11+00.05 MM1
- A multi-transition molecular line study of infrared dark cloud G331.71+00.59
- Herschel Observations of a Newly Discovered UX Ori Star in the Large Magellanic Cloud
- UV Spectropolarimetry with Polstar: Protoplanetary Disks
- Time variability in the bipolar scattered light nebula of L1527 IRS: A possible warped inner disk
- Candidate Coronagraphic Detections of Protoplanetary Disks around Four Young Stars
- Star formation in the luminous YSO IRAS 18345-0641
- Mid-infrared interferometry of massive young stellar objects
- The accretion luminosity of Class I protostars
- The Nature of Class I Sources: Periodic Variables in Orion
- Herschel Far IR observations of the giant HII region NGC 3603
- Photometric variability of the pre-main sequence stars towards the Sh 2-190 region
- Tracking the evolutionary stage of protostars by the abundances of astrophysical ices
- Panchromatic radiation from galaxies as a probe of galaxy formation and evolution
- Discovery of two embedded massive YSOs and an outflow in IRAS 18144-1723
- Observational characteristics of dense cores with deeply embedded young protostars
- The Power of SOFIA/FORCAST in Estimating Internal Luminosities of Low Mass Class 0/I Protostars
- Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): V721 CrA and BN CrA have wide and structured disks in polarised IR
- Semi-analytic calculations for extended mid-Infrared emission associated with FU Ori-type objects
- YSO search toward the boundary of the Central Molecular Zone with near-infrared polarimetry
- Multiple outflows from the luminous YSO IRAS 07422-2001
- A framework for modeling the evolution of young stellar objects
- Why are accreting T Tauri stars less luminous in X-rays than non-accretors?
- Oxyster: A Circumgalactic Low-ionization Oxygen Nebula next to a Starburst Galaxy at
- Star Formation at milli-arcsecond resolution
- Linking Young Stellar Object Morphology to Evolutionary Stages with Self-Organizing Maps