SIMBAD references

2012ApJ...759...47S - Astrophys. J., 759, 47 (2012/November-1)

Observational constraints on the stellar radiation field impinging on transitional disk atmospheres.

SZULAGYI J., PASCUCCI I., ABRAHAM P., APAI D., BOUWMAN J. and MOOR A.

Abstract (from CDS):

Mid-infrared atomic and ionic line ratios measured in spectra of pre-main-sequence stars are sensitive indicators of the hardness of the radiation field impinging on the disk surface. We present a low-resolution Spitzer IRS search for [Ar II] at 6.98 µm, [Ne II] at 12.81 µm, and [Ne III] 15.55 µm lines in 56 transitional disks. These objects, characterized by reduced near-infrared but strong far-infrared excess emission, are ideal targets to set constraints on the stellar radiation field onto the disk, because their spectra are not contaminated by shock emission from jets/outflows or by molecular emission lines. After demonstrating that we can detect [Ne II] lines and recover their fluxes from the low-resolution spectra, here we report the first detections of [Ar II] lines toward protoplanetary disks. We did not detect [Ne III] emission in any of our sources. Our [Ne II]/[Ne III] line flux ratios combined with literature data suggest that a soft-EUV or X-ray spectrum produces these gas lines. Furthermore, the [Ar II]/[Ne II] line flux ratios point to a soft X-ray and/or soft-EUV stellar spectrum as the ionization source of the [Ar II] and [Ne II] emitting layer of the disk. If the soft X-ray component dominates over the EUV, then we would expect larger photoevaporation rates and, hence, a reduction of the time available to form planets.

Abstract Copyright:

Journal keyword(s): circumstellar matter - infrared: stars - protoplanetary disks - stars: pre-main sequence

Simbad objects: 82

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2019.10.14-06:47:16

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