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Related papers: 3D Spectroscopy of Herbig-Haro objects

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We present a detailed analysis of the extended structure detected around the young and close-by Herbig Ae/Be star RCrA. This is a young triple system with an intermediate mass central binary whose separation is of the order of a few tens of…

Low radio frequencies are favourable for the identification of emission from non-thermal processes such as synchrotron emission. The massive protostellar jet associated with IRAS 18162-2048 (also known as the HH80-81 system) has been imaged…

Solar and Stellar Astrophysics · Physics 2017-12-27 S. Vig , V. S. Veena , S. Mandal , A. Tej , S. K. Ghosh

HD163296 is a Herbig Ae star which drives a bipolar knotty jet with a total length of ~6000au. Strong evidence exists that the disk of HD163296 harbors planets. Studies have shown that the presence of companions around jet-driving stars…

Solar and Stellar Astrophysics · Physics 2022-07-13 A. Kirwan , A. Murphy , P. C Schneider , E. T. Whelan , C. Dougados , J. Eislöffel

It has been recently discovered that spatially separated Herbig-Haro objects, once considered unrelated, are linked within a chain that may extend for parsecs in either direction of the embedded protostar forming a "giant Herbig-Haro jet".…

Astrophysics · Physics 2016-08-30 Elisabete M. de Gouveia Dal Pino

We present near-infrared [Fe II] images of four Class 0/I jets (HH 1/2, HH 34, HH 111, HH 46/47) observed with the Hubble Space Telescope Wide Field Camera 3. The unprecedented angular resolution allows us to measure proper motions, jet…

We present 3D, gasdynamic simulations of jet/cloud collisions, with the purpose of modelling the HH 270/110 system. From the models, we obtain predictions of H$\alpha$ and H$_2$ 1-0 s(1) emission line maps, which qualitatively reproduce…

We present the results of a photographic and CCD imaging survey for Herbig-Haro (HH) objects in the L1630 and L1641 giant molecular clouds in Orion. The new HH flows were initially identified from a deep H-alpha film from the recently…

Astrophysics · Physics 2009-10-31 S. L. Mader , W. J. Zealey , Q. A. Parker , M. R. W. Masheder

We have carried out an extensive observational study (from BIMA data) and made a preliminary theoretical investigation of the molecular gas around HH2. The molecular maps show a very complex morphological, kinematical and chemical…

Astrophysics · Physics 2009-11-11 J. M. Girart , S. Viti , R. Estalella , D. A. Williams

HH 212 is a highly collimated jet discovered in H2 powered by a young Class 0 source, IRAS 05413-0104, in the L1630 cloud of Orion. We have mapped around it in 1.33 mm continuum, 12CO ($J=2-1$), 13CO ($J=2-1$), C18O ($J=2-1$), and SO ($J_K…

The shapes of jets with transverse energies, E_T(jet), up to 45 GeV produced in neutral- and charged-current deep inelastic e+p scattering (DIS) at Q**2 > 100 GeV**2 have been measured with the ZEUS detector at HERA. Jets are identified…

High Energy Physics - Experiment · Physics 2012-08-27 ZEUS Collaboration

We present far-ultraviolet (UV) observations at 150 nm of the jet of the quasar 3C 273 obtained with the Advanced Camera for Survey's Solar Blind Channel (ACS/SBC) on board the Hubble Space Telescope. While the jet morphology is very…

Astrophysics · Physics 2014-11-18 Sebastian Jester , Klaus Meisenheimer , Andre' Martel , Eric Perlman , Bill Sparks

Many jets exhibit twisted helical structures. Where superluminal motions are detected, jet orientation and pattern/flow speed are considerably constrained. In this case modeling efforts can place strong limits on conditions in the jet and…

Astrophysics · Physics 2009-11-10 P. E. Hardee

The proto-planetary nebula Hen 3-1475 shows a remarkable highly collimated optical jet with an S-shaped string of three pairs of knots and extremely high velocities. We present here a detailed analysis of the overall morphology, kinematic…

Astrophysics · Physics 2011-05-23 A. Riera , P. Garcia-Lario , A. Manchado , M. Bobrowsky , R. Estalella

The remarkable stability of extragalactic jets is surprising, given the reasonable possibility of the growth of instabilities. In addition, much work in the literature has invoked this possibility in order to explain observed jet structures…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Manel Perucho , Iván Martí-Vidal , Andrei P. Lobanov , Philip E. Hardee

Recent high-resolution high-sensitivity observations of protostellar jets have shown many to possess deviations to their trajectories. HH 211 is one such example where sub-mm observations with the SMA have revealed a clear…

Solar and Stellar Astrophysics · Physics 2016-05-25 Anthony Moraghan , Chin-Fei Lee , Po-Sheng Huang , Bhargav Vaidya

We have identified a new externally irradiated Herbig-Haro (HH) jet, HH 1158, within ~2 pc of the massive OB type stars in the sigma Orionis cluster. At an Lbol ~ 0.1 Lsun, HH 1158 is the lowest luminosity irradiated HH jet identified to…

Solar and Stellar Astrophysics · Physics 2015-12-23 B. Riaz , E. T. Whelan

We present results from a study of molecular gas and dust in the vicinity of the Herbig Haro object HH2. Emission from the sub-mm continuum, 12CO and HCO+ was mapped with angular resolutions ranging from 14 arcsec to 5 arcsec (or 0.01pc at…

Astrophysics · Physics 2009-11-07 W. R. F. Dent , R. S. Furuya , C. J. Davis

A measurement is presented of dijet and 3-jet cross sections in low-|t| diffractive deep-inelastic scattering interactions of the type ep -> eXY, where the system X is separated by a large rapidity gap from a low-mass baryonic system Y.…

High Energy Physics - Experiment · Physics 2008-11-26 H1 Collaboration , C. Adloff

We present results based on the first 20 Chandra images obtained in a survey of jets in radio selected flat-spectrum quasars (FSRQs), along with new sub-arcsecond radio maps and optical images. We discover jet X-ray flux in 12 sources…

The complete near infrared (0.9-2.5 micron) spectra in three different star forming regions (HH24-26, HH72 and BHR71) are presented and analyzed in the framework of shock excitation models. The spectra are dominated by H_2 rovibrational…

Astrophysics · Physics 2009-11-10 T. Giannini , C. McCoey , A. Caratti o Garatti , B. Nisini , D. Lorenzetti , D. R. Flower
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