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相关论文: A search for disks around massive young stellar ob…

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We present a sensitive, multiwavelength submillimeter continuum survey of 153 young stellar objects in the Taurus-Auriga star formation region. The submillimeter detection rate is 61% to a completeness limit of ~10 mJy (3-sigma) at 850…

天体物理学 · 物理学 2008-11-26 Sean M. Andrews , Jonathan P. Williams

We present new results from the Disks@EVLA program for two young stars: CY Tau and DoAr 25. We trace continuum emission arising from their circusmtellar disks from spatially resolved observations, down to tens of AU scales, at {\lambda} =…

We present 7-mm continuum observations of 14 low-mass pre-main-sequence stars in the Taurus-Auriga star-forming region obtained with the Very Large Array with ~1.5" resolution and ~0.3 mJy rms sensitivity. For 10 objects, the circumstellar…

天体物理学 · 物理学 2009-11-11 J. Rodmann , Th. Henning , C. J. Chandler , L. G. Mundy , D. J. Wilner

(Abridged) We present results from a JCMT/SCUBA 850 um search for cold dust around nearby young stars belonging to the beta Pic (t~12 Myr) and the Local Association (t~50 Myr) moving groups. Unlike most past sub-mm studies, our sample was…

天体物理学 · 物理学 2009-11-10 Michael C. Liu , Brenda C. Matthews , Jonathan P. Williams , Paul G. Kalas

We present multi-wavelengths observations and a radiative transfer model of a newly discovered massive circumstellar disk of gas and dust which is one of the largest disks known today. Seen almost edge-on, the disk is resolved in…

This contribution reviews results from interferometric observations of circumstellar disks around young stars of $\lesssim$3 M$_{\odot}$, performed with the MIDI instrument operating in the 10 $\mu$m spectral region. Two main topics, the…

天体物理学 · 物理学 2009-11-13 Roy van Boekel

We present Karl G. Jansky Very Large Array (VLA) observations of the 7 mm continuum emission from the disk surrounding the young star LkCa 15. The observations achieve an angular resolution of 70 mas and spatially resolve the circumstellar…

地球与行星天体物理 · 物理学 2015-06-19 Andrea Isella , Claire J. Chandler , John M. Carpenter , Laura M. Pe'rez , Luca Ricci

We present a detailed analysis for a subset of the high resolution (~35 mas, or 5 au) ALMA observations from the Disk Substructures at High Angular Resolution Project (DSHARP) to search for faint 1.3 mm continuum emission associated with…

We present ALMA observations of the Orion Nebula that cover the OMC1 outflow region. Our focus in this paper is on compact emission from protoplanetary disks. We mosaicked a field containing $\sim 600$ near-IR-identified young stars, around…

太阳与恒星天体物理 · 物理学 2016-07-20 J. A. Eisner , J. M. Bally , A. Ginsburg , P. D. Sheehan

We present 870 micron observations of dust continuum emission from the LkCa 15 protoplanetary disk at high angular resolution (with a characteristic scale of 0.25" = 35 AU), obtained with the IRAM Plateau de Bure interferometer and…

地球与行星天体物理 · 物理学 2015-05-30 Sean M. Andrews , Katherine A. Rosenfeld , David J. Wilner , Michael Bremer

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 $J = 3 - 2$…

地球与行星天体物理 · 物理学 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 observations with the Submillimeter Array of the continuum emission at $\lambda = 1.3$ mm from 62 young stars surrounded by a protoplanetary disk in the Serpens star-forming region. The typical angular resolution for the survey…

星系天体物理 · 物理学 2017-12-13 Charles J. Law , Luca Ricci , Sean M. Andrews , David J. Wilner , Chunhua Qi

Circumstellar disks around stars older than 10 Myr are expected to be gas-poor. There are, however, two examples of old (30-40 Myr) debris-like disks containing a detectable amount of cold CO gas. Here we present ALMA and Herschel Space…

太阳与恒星天体物理 · 物理学 2015-06-17 A. Moór , A. Juhász , Á. Kóspál , P. Ábrahám , D. Apai , T. Csengeri , C. Grady , Th. Henning , A. M. Hughes , Cs. Kiss , I. Pascucci , M. Schmalzl , K. Gabányi

Sub-arcsecond scale Keck images of the young A1V star, 49 Ceti, resolve emission at lambda = 12.5 and 17.9 microns from a disk with long axis at PA 125 pm 10 degrees and inclination phi = 60 pm 15 degrees . At 17.9 microns, the emission is…

天体物理学 · 物理学 2008-11-26 Z. Wahhaj , D. W. Koerner , A. I. Sargent

We present the first observational confirmation for an extended circumstellar dust disk around epsilon Eri. The observations were obtained with the bolometer array SIMBA at the 15 m radio telescope SEST in Chile and measure the dust…

天体物理学 · 物理学 2009-11-10 O. Schuetz , M. Nielbock , S. Wolf , Th. Henning , S. Els

We present the discovery of a spatially unresolved source of sub-millimeter continuum emission ($\lambda=855$ $\mu$m) associated with a young planet, PDS 70 c, recently detected in H$\alpha$ emission around the 5 Myr old T Tauri star PDS…

地球与行星天体物理 · 物理学 2019-07-17 Andrea Isella , Myriam Benisty , Richard Teague , Jaehan Bae , Miriam Keppler , Stefano Facchini , Laura M Pérez

We present ALMA observations of the GQ Lup system, a young Sun-like star with a substellar mass companion in a wide-separation orbit. These observations of 870 $\mu$m continuum and CO J=3-2 line emission with beam size $\sim0.3''$ ($\sim45$…

We have observed 22 Lindroos stars with SCUBA on the JCMT to search for evidence of dust discs. Stars in this sample are the less massive companions of B-type primaries and have ages of 10-170Myr. Dust was detected around three of these…

天体物理学 · 物理学 2009-11-07 M. C. Wyatt , W. R. F. Dent , J. S. Greaves

We report on observations of circumstellar disks around young stars that have been obtained with the MIDI instrument, which is mounted on the VLT Interferometer and operates in the 10 micrometer atmospheric window. The maximum spatial…

We present ALMA observations of the 0.88 millimeter dust continuum, 13CO, and C18O J=3-2 line emission of the circumbinary disk HD142527 at a spatial resolution of about 0.25". This system is characterized by a large central cavity of…

地球与行星天体物理 · 物理学 2017-05-10 Y. Boehler , E. Weaver , A. Isella , L. Ricci , C. Grady , J. Carpenter , L. Perez
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