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HD141569 is a pre-main sequence star with a disc uniquely placed between protoplanetary and debris discs, similar to the older `hybrid' type discs. This work aims to place the mass and spatial structure of the disc midplane in the context…

Earth and Planetary Astrophysics · Physics 2018-07-25 James Miley , Olja Panic , Mark Wyatt , Grant Kennedy

Gas-rich primordial disks and tenuous gas-poor debris disks are usually considered as two distinct evolutionary phases of the circumstellar matter. Interestingly, the debris disk around the young main-sequence star 49 Ceti possesses a…

Solar and Stellar Astrophysics · Physics 2015-05-30 A. Moór , P. Ábrahám , A. Juhász , Cs. Kiss , I. Pascucci , Á. Kóspál , D. Apai , Th. Henning , T. Csengeri , C. Grady

Maps and measurements of the J=1-0, J=2-1, J=3-2, J=4-3 12CO, the J=1-0, J=2-1, and J=3-2 13CO lines in the central arcminute squared of NGC1068, NGC2146, NGC3079, NGC4826, and NGC7469, as well as 492 GHz [CI] maps in three of these are…

Astrophysics · Physics 2009-11-13 F. P. Israel

The results of single-dish observations of low- and high-J transitions of selected molecules from protoplanetary disks around two TTauri stars (LkCa15 and TWHya) and two HerbigAe stars (HD163296 and MWC480) are reported. Simple molecules…

Astrophysics · Physics 2011-07-18 Wing-Fai Thi , Gerd-Jan van Zadelhoff , Ewine F. van Dishoeck

Debris disks are usually detected through the infrared excess over the photospheric level of their host star. The most favorable stars for disk detection are those with spectral types between A and K, while the statistics for debris disks…

We present new high-quality ALMA observations of the Red Rectangle (a well known post-AGB object) in C17O J=6-5 and H13CN J=4-3 line emission and results from a new reduction of already published 13CO J=3-2 data. A detailed model fitting of…

Solar and Stellar Astrophysics · Physics 2016-10-05 V. Bujarrabal , A. Castro-Carrizo , J. Alcolea , M. Santander-Garcia , H. Van Winckel , C. Sanchez Contreras

We present high angular resolution (0.5-2.0") observations of the mm continuum and the 12CO(J=3-2), 13CO(J=3-2), 13CO(J=2-1), C18O(J=2-1), HCN(J=3-2), HCO+(J=4-3) and HCO+(J=3-2) line emission in the circumnuclear disk (r=100pc) of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 M. Krips , S. Martin , A. Eckart , R. Neri , S. Garcia-Burillo , S. Matsushita , A. Peck , I. Stoklasova , G. Petitpas , A. Usero , F. Combes , E. Schinnerer , L. Humphreys , A. J. Baker

HD 141569 is a Herbig Ae/Be star that straddles the boundary between the transition disks and debris disks. It is a low dust mass disk that reveals numerous structural elements (e.g. gaps and rings) that may point to young planets. It also…

Solar and Stellar Astrophysics · Physics 2021-12-16 Stanley K. Jensen , Sean D. Brittain , Joan R. Najita , John S. Carr

Using the IRAM 30m telescope, we have surveyed an unbiased sample of 47 nearby spiral galaxies of very late (Scd-Sm) Hubble-type for emission in the CO(1-0) and CO(2-1) lines. The sensitivity of our data (a few mK) allows detection of about…

Astrophysics · Physics 2009-11-07 T. Boeker , U. Lisenfeld , E. Schinnerer

The formation process of massive stars is not well understood, and advancement in our understanding benefits from high resolution observations and modelling of the gas and dust surrounding individual high-mass (proto)stars. Here we report…

Solar and Stellar Astrophysics · Physics 2016-08-22 J. D. Ilee , C. J. Cyganowski , P. Nazari , T. R. Hunter , C. L. Brogan , D. H. Forgan , Q. Zhang

We report the detection of CO(1-0) and CO(2-1) emission from the central region of nearby 3CR radio galaxies (z$<$ 0.03). Out of 21 galaxies, 8 have been detected in, at least, one of the two CO transitions. The total molecular gas content…

Astrophysics · Physics 2009-09-25 S. Leon , J. Lim , F. Combes , D. Van-Trung

The Kepler extended mission, also known as K2, has provided the community with a wealth of planetary candidates that orbit stars typically much brighter than the targets of the original mission. These planet candidates are suitable for…

Deep HST broad-band images taken with ACS and WFPC2 of the giant ($\sim 1000$ AU diameter) dark silhouette proplyd 114-426 in the Orion Nebula show that this system is tilted, asymmetric, warped and photoevaporated. The exquisite angular…

Solar and Stellar Astrophysics · Physics 2016-03-02 Anna Miotello , Massimo Robberto , Marco A. C. Potenza , Luca Ricci

We present an ACA search for [CI] emission at 492GHz toward large T Tauri disks (gas radii $\gtrsim 200$au) in the $\sim 1-3$Myr-old Lupus star-forming region. Combined with ALMA 12-m archival data for IM Lup, we report [CI] detections in 6…

We present new 10.8 and 18.2 micron images of HR 4796A, a young A0V star that was recently discovered to have a spectacular, nearly edge-on, circumstellar disk prominent at ~20 microns (Jayawardhana et al. 1998; Koerner et al. 1998). These…

The circumstellar disk of AB Aurigae has garnered strong attention owing to the apparent existence of spirals at a relatively young stage and also the asymmetric disk traced in thermal dust emission. However, the physical conditions of the…

Astrophysics of Galaxies · Physics 2015-06-11 Ya-Wen Tang , Stephane Guilloteau , Vincent Pietu , Anne Dutrey , Nagayoshi Ohashi , Paul T. P. Ho

We present new 0.6 - 4 $\mu$m imaging of the SR 21 transition disk from Keck/NIRC2 and Magellan/MagAO. The protoplanetary disk around SR 21 has a large (~ 30 - 40 AU) clearing first inferred from its spectral energy distribution and later…

We present Keck/OSIRIS 1.1-1.8 um adaptive optics integral field spectroscopy of the planetary-mass companion to GSC 06214-00210, a member of the ~5 Myr Upper Scorpius OB association. We infer a spectral type of L0+/-1, and our spectrum…

Earth and Planetary Astrophysics · Physics 2015-05-30 Brendan P. Bowler , Michael C. Liu , Adam L. Kraus , Andrew W. Mann , Michael J. Ireland

We present ALMA observations of the 2M1207 system, a young binary made of a brown dwarf with a planetary-mass companion at a projected separation of about 40 au. We detect emission from dust continuum at 0.89 mm and from the $J = 3 - 2$…

Earth and Planetary Astrophysics · Physics 2017-07-05 L. Ricci , P. Cazzoletti , I. Czekala , S. Andrews , D. Wilner , L. Szucs , G. Lodato , L. Testi , I. Pascucci , S. Mohanty , D. Apai , J. Carpenter , B. Bowler

We present ALMA observations of CO $J = 2-1$ and CS $J = 5-4$ emission from the disk around TW~Hydrae. Both molecules trace a predominantly Keplerian velocity structure, although a slowing of the rotation velocity is detected at the outer…