Lack of PAH emission toward low-mass embedded young stellar objects

Abstract

PAHs have been detected toward molecular clouds and some young stars with disks, but have not yet been associated with embedded young stars. We present a sensitive mid-IR spectroscopic survey of PAH features toward a sample of low-mass embedded YSOs. The aim is to put constraints on the PAH abundance in the embedded phase of star formation using radiative transfer modeling. VLT-ISAAC L-band spectra for 39 sources and Spitzer IRS spectra for 53 sources are presented. Line intensities are compared to recent surveys of Herbig Ae/Be and T Tauri stars. The radiative transfer codes RADMC and RADICAL are used to model the PAH emission from embedded YSOs consisting of a PMS star with a circumstellar disk embedded in an envelope. The dependence of the PAH feature on PAH abundance, stellar radiation field, inclination and the extinction by the surrounding envelope is studied. The 3.3 micron PAH feature is undetected for the majority of the sample (97%), with typical upper limits of 5E-16 W/m^2. Compact 11.2 micron PAH emission is seen directly towards 1 out of the 53 Spitzer Short-High spectra, for a source that is borderline embedded. For all 12 sources with both VLT and Spitzer spectra, no PAH features are detected in either. In total, PAH features are detected toward at most 1 out of 63 (candidate) embedded protostars (<~ 2%), even lower than observed for class II T Tauri stars with disks (11-14%). Assuming typical class I stellar and envelope parameters, the absence of PAHs emission is most likely explained by the absence of emitting carriers through a PAH abundance at least an order of magnitude lower than in molecular clouds but similar to that found in disks. Thus, most PAHs likely enter the protoplanetary disks frozen out in icy layers on dust grains and/or in coagulated form.

13 pages, 9 figures, accepted for publication in A&A

References in corpus (12)

• The Evolution of Outflow-Envelope Interactions in Low-Mass Protostars
• The c2d Spitzer spectroscopic survey of ices around low-mass young stellar objects II: CO2
• The Stellar Population of the Chamaeleon I Star-Forming Region
• The origin of hydrogen line emission for five Herbig Ae/Be stars spatially resolved by VLTI/AMBER spectro-interferometry
• Current Star Formation in the Ophiuchus and Perseus Molecular Clouds: Constraints and Comparisons from Unbiased Submillimeter and Mid-Infrared Surveys. II
• c2d Spitzer IRS Spectra of Disks around T Tauri Stars. III. [Ne II], [Fe I], and H_2 gas-phase lines
• Characterizing the nature of embedded young stellar objects through silicate, ice and millimeter observations
• Spatially extended PAHs in circumstellar disks around T Tauri and Herbig Ae stars
• PAH chemistry and IR emission from circumstellar disks
• Spitzer-IRS spectra of disks around T Tauri stars II. PAH emission features
• Spatial separation of small and large grains in the transitional disk around the young star IRS 48
• Modeling the gas-phase chemistry of the transitional disk around HD 141569A

Cited by in corpus (1)

• Formation of Water in the Warm Atmospheres of Protoplanetary Disks