TY - JOUR
T1 - Constraining the structure of the transition disk HD 135344B (SAO 206462) by simultaneous modeling of multiwavelength gas and dust observations
AU - Carmona, A.
AU - Pinte, C.
AU - Thi, W.F.
AU - Benisty, M.
AU - Ménard, F.
AU - Grady, C.
AU - Kamp, I.
AU - Woitke, P.
AU - Olofsson, J.
AU - Roberge, A.
AU - Brittain, S.
AU - Duchêne, G.
AU - Meeus, G.
AU - Martin-Zaïdi, C.
AU - Dent, B.
AU - Le Bouquin, J.B.
AU - Berger, J.P.
PY - 2014/7/10
Y1 - 2014/7/10
N2 - Context. Constraining the gas and dust disk structure of transition disks, particularly in the inner dust cavity, is a crucial step toward understanding the link between them and planet formation. HD 135344B is an accreting (pre-)transition disk that displays the CO 4.7 μm emission extending tens of AU inside its 30 AU dust cavity. Aims. We constrain HD 135344B's disk structure from multi-instrument gas and dust observations. Methods. We used the dust radiative transfer code MCFOST and the thermochemical code ProDiMo to derive the disk structure from the simultaneous modeling of the spectral energy distribution (SED), VLT/CRIRES CO P(10) 4.75 μm, Herschel/PACS [OI] 63 μm, Spitzer/IRS, and JCMT 12CO J = 3-2 spectra, VLTI/PIONIER H-band visibilities, and constraints from (sub-)mm continuum interferometry and near-IR imaging. Results. We found a disk model able to describe the current gas and dust observations simultaneously.
AB - Context. Constraining the gas and dust disk structure of transition disks, particularly in the inner dust cavity, is a crucial step toward understanding the link between them and planet formation. HD 135344B is an accreting (pre-)transition disk that displays the CO 4.7 μm emission extending tens of AU inside its 30 AU dust cavity. Aims. We constrain HD 135344B's disk structure from multi-instrument gas and dust observations. Methods. We used the dust radiative transfer code MCFOST and the thermochemical code ProDiMo to derive the disk structure from the simultaneous modeling of the spectral energy distribution (SED), VLT/CRIRES CO P(10) 4.75 μm, Herschel/PACS [OI] 63 μm, Spitzer/IRS, and JCMT 12CO J = 3-2 spectra, VLTI/PIONIER H-band visibilities, and constraints from (sub-)mm continuum interferometry and near-IR imaging. Results. We found a disk model able to describe the current gas and dust observations simultaneously.
KW - Protoplanetary disks
KW - Stars: pre-main sequence
KW - Planets and satellites: formation
KW - Techniques: high angular resolution
KW - Techniques: interferometric
KW - Stars: individual: HD 135344B (SAO 206462)
U2 - 10.1051/0004-6361/201322534
DO - 10.1051/0004-6361/201322534
M3 - Article
AN - SCOPUS:84903958313
SN - 0004-6361
VL - 567
JO - Astronomy & Astrophysics
JF - Astronomy & Astrophysics
M1 - A51
ER -