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In this study, we present high-resolution millimeter observations of the dust and gas disk of the T Tauri star AS 205 N and its companion, AS 205 S, obtained with the Atacama Large Millimeter Array. The gas disk around AS 205 N, for which…

太阳与恒星天体物理 · 物理学 2015-06-22 Colette Salyk , Klaus Pontoppidan , Stuartt Corder , Diego Muñoz , Ke Zhang , Geoffrey A. Blake

Infrared observations of the inner disks around very low-mass stars (VLMS, $<$0.3$\,M_{\odot}$) have revealed a carbon-rich gas composition in the terrestrial planet-forming regions. Contrary to the typically water-rich T Tauri disk…

Observations from Spitzer and ground-based infrared spectroscopy reveal significant diversity in the molecular emission from the inner few AU of T Tauri disks. We explore theoretically the possible origin of this diversity by expanding on…

太阳与恒星天体物理 · 物理学 2015-05-30 Joan R. Najita , Mate Adamkovics , Alfred E. Glassgold

Millimeter observations of CO isotopologues are often used to make inferences about protoplanetary disk gas density and temperature structures. The accuracy of these estimates depends on our understanding of CO freezeout and desorption from…

太阳与恒星天体物理 · 物理学 2016-06-01 Jane Huang , Karin I. Oberg , Sean M. Andrews

The evolution of planet-forming regions in protoplanetary disks is of fundamental importance to understanding planet formation. Disks with a central deficit in dust emission, a "cavity", have long attracted interest as potential evidence…

Most stars form in multiple systems whose properties can significantly impact circumstellar disk evolution. We investigate the physical and chemical properties of the equal-mass, small separation (~66 mas, ~9 au) DF Tau binary system.…

We present high resolution (R = 100,000) L-band spectroscopy of 11 Herbig AeBe stars with circumstellar disks. The observations were obtained with the VLT/CRIRES to detect hot water and hydroxyl radical emission lines previously detected in…

太阳与恒星天体物理 · 物理学 2015-05-27 D. Fedele , I. Pascucci , S. Brittain , I. Kamp , P. Woitke , J. P. Williams , W. R. F. Dent , W. -F. Thi

Theoretical models and observations suggest that the abundances of molecular ions in protoplanetary disks should be highly sensitive to the variable ionization conditions set by the young central star. We present a search for temporal flux…

We investigate which properties of protoplanetary disks around T Tauri stars affect the physics and chemistry in the regions where mid- and far-IR water lines originate and their respective line fluxes. We search for diagnostics for future…

太阳与恒星天体物理 · 物理学 2021-06-04 S. Antonellini , I. Kamp , P. Riviere-Marichalar , R. Meijerink , P. Woitke , W. -F. Thi , M. Spaans , G. Aresu , E. K. H. Lee

The unstable accretion phases during pre-main-sequence evolution of T Tauri stars produce variable irradiation and heating of planet-forming regions. A strong accretion outburst was observed with Spitzer-IRS in 2008 in EX Lup, the prototype…

We observed the Herbig Ae/Be stars UX Ori, HD 34282, HD 100453, HD 101412, HD 104237 and HD 142666, and the T Tauri star HD 319139 and searched for H2 0-0 S(2) emission at 12.278 micron and H2 0-0 S(1) emission at 17.035 micron with VISIR,…

We present a MIRI-MRS spectrum of the high-inclination protoplanetary disk around the solar-mass (K0) star MY Lup, obtained as part of the JWST Disk Infrared Spectral Chemistry Survey (JDISCS). The spectrum shows an unusually weak water…

We present a new velocity-resolved survey of 2.9 $\mu$m spectra of hot H$_2$O and OH gas emission from protoplanetary disks, obtained with CRIRES at the VLT ($\Delta v \sim$ 3 km s$^{-1}$). With the addition of archival Spitzer-IRS spectra,…

地球与行星天体物理 · 物理学 2017-01-18 A. Banzatti , K. M. Pontoppidan , C. Salyk , G. Herczeg , E. F. van Dishoeck , G. A. Blake

We present an observational reconstruction of the radial water vapor content near the surface of the TW Hya transitional protoplanetary disk, and report the first localization of the snow line during this phase of disk evolution. The…

地球与行星天体物理 · 物理学 2015-06-15 K. Zhang , K. M. Pontoppidan , C. Salyk , G. A. Blake

As part of the JWST GTO program MINDS, we analyze the mid-infrared emission of three Class II binary systems: VW Cha, WX Cha, and RW Aur, to investigate the impact of stellar multiplicity on the chemistry and physics of their inner disk. We…

Circumstellar disks provide the material reservoir for the growth of young stars and for planet formation. We combine a high-level radiative transfer program with a thermal-chemical model of a typical T Tauri star disk to investigate the…

天体物理学 · 物理学 2009-11-13 R. Meijerink , D. R. Poelman , M. Spaans , A. G. G. M. Tielens , A. E. Glassgold

We report on the observation of hot water vapor (steam) in the inner AU of a young massive star located in the star-forming region IRAS 08576-4334. The water lines are detected in a medium resolution (R=10,000) K-band spectrum taken by the…

天体物理学 · 物理学 2009-11-10 W. -F. Thi , A. Bik

(Abridged) Rotational H$_2$O spectra as observed with JWST/MIRI provide a good probe of the temperature and column density structure of the inner disk. H$_2$O emission can also be influenced by dynamical processes, such as dust grains…

地球与行星天体物理 · 物理学 2025-11-05 Marissa Vlasblom , Milou Temmink , Andrew D. Sellek , Ewine F. van Dishoeck

We present an analysis of high-resolution spectroscopy of several bright T Tauri stars using the VLT/CRIRES and Keck/NIRSPEC spectrographs, revealing the first detections of emission from HCN and C2H2 in circumstellar disks at near-infrared…

地球与行星天体物理 · 物理学 2015-06-03 A. M. Mandell , J. Bast , E. F. van Dishoeck , G. A. Blake , C. Salyk , M. J. Mumma , G. Villanueva