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Full Record Details
Persistent URL
http://purl.org/net/epubs/work/10775761
Record Status
Checked
Record Id
10775761
Title
Gas lines from the 5-Myr old optically thin disk around HD141569A. Herschel observations and modeling
Contributors
W-F Thi
,
C Pinte
,
E Pantin
,
J-C Augereau
,
G Meeus
,
F Menard
,
C Martin-Zaidi
,
P Woitke
,
P Riviere-Marichalar
,
I Kamp
,
A Carmona
,
G Sandell
,
C Eiroa
,
W Dent
,
B Montesinos
,
G Aresu
,
R Meijerink
,
M Spaans
,
G White (STFC Rutherford Appleton Lab., and The Open Univ.)
,
D Ardila
,
J Lebreton
,
I Mendigutia
,
S Brittain
Abstract
At the distance of 99-116 pc, HD141569A is one of the nearest HerbigAe stars that is surrounded by a tenuous disk, probably in transition between a massive primordial disk and a debris disk. We observed the fine-structure lines of OI at 63 and 145 micron and the CII line at 157 micron with the PACS instrument onboard the Herschel Space Telescope as part of the open-time large programme GASPS. We complemented the atomic line observations with archival Spitzer spectroscopic and photometric continuum data, a ground-based VLT-VISIR image at 8.6 micron, and 12CO fundamental ro-vibrational and pure rotational J=3-2 observations. We simultaneously modeled the continuum emission and the line fluxes with the Monte Carlo radiative transfer code MCFOST and the thermo-chemical code ProDiMo to derive the disk gas- and dust properties assuming no dust settling. The models suggest that the oxygen lines are emitted from the inner disk around HD141569A, whereas the [CII] line emission is more extended. The CO submillimeter flux is emitted mostly by the outer disk. Simultaneous modeling of the photometric and line data using a realistic disk structure suggests a dust mass derived from grains with a radius smaller than 1 mm of 2.1E-7 MSun and from grains with a radius of up to 1 cm of 4.9E-6 MSun. We constrained the polycyclic aromatic hydrocarbons (PAH) mass to be between 2E-11 and 1..4E-10 MSun assuming circumcircumcoronene (C150H30) as the representative PAH. The associated PAH abundance relative to hydrogen is lower than those found in the interstellar medium (3E-7) by two to three orders of magnitude. The disk around HD141569A is less massive in gas (2.5 to 4.9E-4 MSun or 67 to 164 MEarth) and has a flat opening angle (<10%). [abridged]
Organisation
STFC
,
RALSP
Keywords
Funding Information
Related Research Object(s):
11872514
Licence Information:
Language
English (EN)
Type
Details
URI(s)
Local file(s)
Year
Preprint
Astron Astrophys
2013.
http://arxiv.org/abs/1309.5098
2013
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