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相关论文: SMA Submillimeter Observations of HL Tau: Revealin…

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We present detailed geometry and kinematics of the inner outflow toward HL Tau observed using Near Infrared Integral Field Spectograph (NIFS) at the Gemini-North 8-m Observatory. We analyzed H2 2.122 um emission and [Fe II] 1.644 um line…

天体物理学 · 物理学 2009-11-13 Michihiro Takami , Tracy L. Beck , Tae-Soo Pyo , Peter McGregor , Christopher Davis

We present Submillimeter Array (SMA) 1.35 mm subarcsecond angular resolution observations toward the LkH{\alpha} 234 intermediate-mass star-forming region. The dust emission arises from a filamentary structure of $\sim$5 arcsec ($\sim$4500…

We present $^{12}$CO(2-1) line and 1300 $\mu$m continuum observations made with the Submillimeter Array (SMA) of the young star DG Tau B. We find, in the continuum observations, emission arising from the circumstellar disk surrounding DG…

太阳与恒星天体物理 · 物理学 2015-06-23 Luis A. Zapata , Susana Lizano , Luis F. Rodriguez , Paul T. P. Ho , Laurent Loinard , Manuel Fernandez-Lopez , Daniel Tafoya

We present Submillimeter Array observations toward the 10^{4.7} Lsun star-forming region G240.31+0.07, in the J=2-1 transition of 12CO and 13CO and at 1.3 mm continuum, as well as the 12CO and 13CO observations from the Caltech…

星系天体物理 · 物理学 2011-02-11 Keping Qiu , Qizhou Zhang , Jingwen Wu , Huei-Ru Chen

Using the Atacama Large Millimeter/submillimeter Array (ALMA), we investigated a peculiar millimeter source MMS 3 located in the Orion Molecular Cloud 3 (OMC-3) region in the 1.3 mm continuum, CO ($J$=2-1), SiO ($J$=5-4), C$^{18}$O…

星系天体物理 · 物理学 2021-04-08 Kaho Morii , Satoko Takahashi , Masahiro N. Machida

We report our SMA observations of the Class \RN{1}-\RN{2} protostar HL Tau in the $^{13}$CO (2--1), C$^{18}$O (2--1), SO(5$_6$--4$_5$), and the 1.3 mm dust-continuum emission and our analyses of the ALMA long baseline data of the HCO$^{+}$…

太阳与恒星天体物理 · 物理学 2018-12-13 Chun-Ju Wu , Naomi Hirano , Shigehisa Takakuwa , Hsi-Wei Yen , Yusuke Aso

We present high angular resolution ($\sim$0.94$"$) $^{12}$CO(1-0) Atacama Large Millimeter/Submillimeter Array (ALMA) observations obtained during the 2014 long baseline campaign from the eruptive bipolar flow from the multiple XZ Tau…

Outflowing motions, whether a wind launched from the disk, a jet launched from the protostar, or the entrained molecular outflow, appear to be an ubiquitous feature of star formation. These outwards motions have a number of root causes, and…

星系天体物理 · 物理学 2016-05-25 Pamela D. Klaassen , Joseph C. Mottram , Luke T. Maud , Attila Juhasz

Using the Submillimeter Array (SMA) on Mauna Kea, the H2-16O 10_2,9-9_3,6 transition (E_up=1863K) at 321.2 GHz has been detected toward the embedded low-mass protostar HL Tau. The line centroid is blue-shifted by 15 km/s with respect to the…

太阳与恒星天体物理 · 物理学 2016-05-25 Lars E. Kristensen , Joanna M. Brown , David Wilner , Colette Salyk

We report the detection of a molecular outflow driven by the brown dwarf binary FU Tau. Using the IRAM 30 m telescope we observed the $^{12}$CO(2-1) (CO) emission in the vicinity of FU Tau and detected a bipolar outflow by examining the…

太阳与恒星天体物理 · 物理学 2015-06-12 J. -L. Monin , E. Whelan , B. Lefloch , C. Dougados , C. Alves de Oliveira

We present interferometric observations in the 12CO (2-1) line and at 1.3 mm dust continuum of the low-mass protostellar binary system in the cometary globule CG30, using the Submillimeter Array. The dust continuum images resolve two…

天体物理学 · 物理学 2009-11-13 Xuepeng Chen , Tyler L. Bourke , Ralf Launhardt , Thomas Henning

DR Tau has been noted for its unusually high variability in comparison with other T Tauri stars. Although it is one of the most extensively studied pre-main sequence stars, observations with millimeter interferometry have so far been…

太阳与恒星天体物理 · 物理学 2023-02-08 Jane Huang , Edwin A. Bergin , Jaehan Bae , Myriam Benisty , Sean M. Andrews

We present 12CO (J=2-1) sensitive molecular line and 1.3 mm continuum observations made with the Submillimeter Array (SMA) of the bipolar outflow associated with the young star located in the Bok globule known as CB 26. The SMA observations…

太阳与恒星天体物理 · 物理学 2023-03-01 J. A. López-Vázquez , Luis A. Zapata , Chin-Fei Lee

We present our observational results of the 1.1 mm continuum and the HCO+ (3-2) line in HL Tau at angular resolutions of 0.1" obtained with ALMA and our data analysis of the 2.9 mm and 1.1 mm continuum and the HCO+ (3-2) and (1-0) lines of…

太阳与恒星天体物理 · 物理学 2019-07-31 Hsi-Wei Yen , Pin-Gao Gu , Naomi Hirano , Patrick M. Koch , Chin-Fei Lee , Hauyu Baobab Liu , Shigehisa Takakuwa

We present new 7 mm and archive 1.3 cm high angular resolution observations of the HL/XZ Tau region made with the VLA. At 7 mm, the emission from HL Tau seems to be arising in a clumpy disk with radius of order 25 AU. The 1.3 cm emission…

太阳与恒星天体物理 · 物理学 2011-02-11 Carlos Carrasco-Gonzalez , Luis F. Rodriguez , Guillem Anglada , Salvador Curiel

The disk-outflow connection is thought to play a key role in extracting excess angular momentum from a forming protostar. We present ALMA 0.25" angular resolution observations - in the dust continuum at 1.33 mm and of the molecular line…

We present high angular-resolution observations of Sakurai's object using the Atacama Large Millimeter Array, shedding new light on its morpho-kinematical structure. The millimetre continuum emission, observed at an angular resolution of 20…

We report here our latest search for molecular outflows from young brown dwarfs and very low-mass stars in nearby star-forming regions. We have observed three sources in Taurus with the Submillimeter Array and the Combined Array for…

太阳与恒星天体物理 · 物理学 2015-06-22 Ngoc Phan-Bao , Chin-Fei Lee , Paul T. P. Ho , Cuong Dang-Duc , Di Li

In this {\it Letter}, we present sensitive millimeter SiO (J=5-4; $\nu$=0) line observations of the outflow arising from the enigmatic object Orion Source I made with the Atacama Large Millimeter/Submillimeter Array (ALMA). The observations…

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