中文
相关论文

相关论文: Monitoring inner regions in the RY Tau jet

200 篇论文

We present new results of [Fe II] 1.644-micron spectroscopy toward the jets from HL Tau and RW Aur carried out with the Subaru Telescope combined with the adaptive optics system. We observed the regions within 2" - 3" from the stars with…

Forbidden neon emission from jets of low-mass young stars can be used to probe the underlying high-energy processes in these systems. We analyze spectra of the jet of DG Tau obtained with the Very Large Telescope/X-Shooter spectrograph in…

太阳与恒星天体物理 · 物理学 2016-12-14 Chun-Fan Liu , Hsien Shang , Gregory J. Herczeg , Frederick M. Walter

Faint X-ray emission from hot plasma (T > 1 MK) has been detected extending outward a few arcseconds along the optically-delineated jets of some classical T Tauri stars including RY Tau. The mechanism and location where the jet is heated to…

太阳与恒星天体物理 · 物理学 2018-04-04 S. L. Skinner , P. C. Schneider , M. Audard , Manuel Guedel

We present survey results which suggest rotation signatures at the base of T-Tauri jets. Observations were conducted with the Hubble Space Telescope Imaging Spectrograph at optical and near ultraviolet wavelengths (NUV). Results are…

天体物理学 · 物理学 2011-02-11 Deirdre Coffey , Francesca Bacciotti , Thomas P. Ray , Jochen Eislöffel , Jens Woitas

First evidences of IR excess and disk mass accretion (strong H$\alpha$ emission) around brown dwarfs seem to indicate the existence of circumstellar disks around these sub-stellar objects. Nothing is known at the present time about outflows…

天体物理学 · 物理学 2009-11-10 E. Masciadri , A. C. Raga

The mechanism and the region of generation of variable continuum emission are poorly understood for radio-loud AGN because of a complexity of the nuclear region. High-resolution radio VLBI (very long baseline interferometry) observations…

宇宙学与河外天体物理 · 物理学 2015-05-14 T. G. Arshakian , J. Leon-Tavares , A. P. Lobanov , V. H. Chavushyan , A. I. Shapovalova , A. N. Burenkov , J. A. Zensus

Jets from young stars represent one of the most striking signposts of star formation. The phenomenon has been researched for over two decades and there is now general agreement that such jets are generated as a by-product of accretion; most…

天体物理学 · 物理学 2007-05-23 Tom Ray , Catherine Dougados , Francesca Bacciotti , Jochen Eisloeffel , Antonio Chrysostomou

We have carried out a spatio-kinematic study of the outflow from the classical T Tauri star DG Tau using the Space Telescope Imaging Spectrograph (STIS) on board the Hubble Space Telescope (HST). A series of seven spatially offset long-slit…

天体物理学 · 物理学 2009-10-31 Francesca Bacciotti , Reinhard Mundt , Thomas P. Ray , Jochen Eisloeffel , Josef Solf , Max Camezind

We present Spitzer (IRAC) images observations and a VLT 2.1micron image of the HH 212 outflow. We find that this outflow has a strong symmetry, with jet/counterjet knot pairs with Delta x less than 1 arcsec position offsets. We deduce that…

天体物理仪器与方法 · 物理学 2020-04-08 A. Noriega-Crespo , A. C. Raga , V. Lora , J. C. Rodriguez-Ramirez , STScI , ICN , UNAM , IRAT , UNAM , IAG , USP

VLA, MERLIN and Hubble Space Telescope imaging observations of the extended regions of the symbiotic system CH Cygni are analysed. These extensions are evidence of a strong collimation mechanism, probably an accretion disk surrounding the…

天体物理学 · 物理学 2009-11-07 M. M. Crocker , R. J. Davis , R. E. Spencer , S. P. S. Eyres , M. F. Bode , A. Skopal

Jets around low- and intermediate-mass young stellar objects (YSOs) contain a fossil record of the recent accretion and outflow activity of their parent star-forming systems. We aim to understand whether the accretion/ejection process is…

太阳与恒星天体物理 · 物理学 2015-06-12 L. E. Ellerbroek , L. Podio , L. Kaper , H. Sana , D. Huppenkothen , A. de Koter , L. Monaco

We report here on the first proper motion measurements of molecular hydrogen emission features in the Herbig-Haro 46/47 outflow. Assuming a distance of 350 pc to this flow, the inferred tangential velocities range from a few tens to almost…

Radio emission in jets from young stellar objects (YSOs) in the form of nonthermal emission has been seen toward several YSOs. Thought to be synchrotron emission from strong shocks in the jet, it could provide valuable information about the…

We present nine epochs of Hubble Space Telescope optical imaging of the bipolar outflow from the pre-main sequence binary XZ Tauri. Our data monitors the system from 1995-2005 and includes emission line images of the flow. The northern lobe…

We present SINFONI/VLT observations of the DG Tauri jet in the [FeII] lines with 0.15" angular resolution and R=3000 spectral resolution. We observe an onion-like velocity structure in [FeII] in the blueshifted jet, similar to that observed…

太阳与恒星天体物理 · 物理学 2015-05-28 V. Agra-Amboage , C. Dougados , S. Cabrit , J. Reunanen

We present near infrared images in H2 at 2.12um of the HH 7/11 outflow and its driving source SVS 13 taken with HST NICMOS 2 camera, as well as archival Ha and [SII] optical images obtained with the WFPC2 camera. The NICMOS high angular…

天体物理学 · 物理学 2009-11-07 A. Noriega-Crespo , A. Cotera , E. Young , H. Chen

We present observations of jets within 2000 au of three deeply embedded protostars using 2.9-27 micron observations with JWST. These observations show the morphologies and kinematics of the collimated jets from three protostars, the…

FS Tau B is one of the few T Tauri stars that possess a jet and a counterjet as well as an optically-visible cavity wall. We obtained images and spectra of its jet-cavity system in the near-infrared H and K bands using Subaru/IRCS and…

We present proper motion measurements of 37 jets and HH objects in the Carina Nebula measured in two epochs of H$\alpha$ images obtained $\sim 10$ yrs apart with HST/ACS. Transverse velocities in all but one jet are faster than $\gtrsim 25$…

太阳与恒星天体物理 · 物理学 2017-08-02 Megan Reiter , Megan M. Kiminki , Nathan Smith , John Bally

Context: IRAS 04166+2706 in Taurus is one of the most nearby young stellar objects whose molecular outflow contains a highly collimated fast component. Methods: We have observed the IRAS 04166+2706 outflow with the IRAM Plateau de Bure…

天体物理学 · 物理学 2009-11-13 J. Santiago-Garcia , M. Tafalla , D. Johnstone , R. Bachiller