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We find strong evidence for outflows originating in the dense molecular core NGC 6334 I(North): a 1000 Msol molecular core distinguished by its lack of HII regions and mid-IR emission. New observations were obtained of the SiO 2-1 and 5-4…

Astrophysics · Physics 2009-10-31 S. T. Megeath , A. R. Tieftrunk

The high spatial and spectral resolution offered by the new generation of infrared spectrometers at ESO is optimally suited for the observational study of outflows from young stellar objects. Models of interstellar shock waves would benefit…

Astrophysics · Physics 2009-11-10 R. Liseau

We have for the first time detected X-ray emission associated with a proto-stellar jet, on the jet emanating from L1551 IRS5. The IRS5 proto-star is hidden beyond a very large absorbing column density, making the direct observation of the…

Astrophysics · Physics 2007-05-23 Fabio Favata , C. V. M. Fridlund , G. Micela , S. Sciortino , A. A. Kaas

We present new near-IR long slit spectroscopic data obtained with ISAAC on VLT/ANTU (ESO/Paranal) of the central 4''x 4'' region surrounding the central engine of NGC1068 . Bracket Gamma (Bg) and H2 emission line maps and line profile grids…

Astrophysics · Physics 2009-11-07 Emmanuel Galliano , Danielle Alloin

HESS J1825-137 is a pulsar wind nebula (PWN) whose TeV emission extends across ~1 deg. Its large asymmetric shape indicates that its progenitor supernova interacted with a molecular cloud located in the north of the PWN as detected by…

High Energy Astrophysical Phenomena · Physics 2016-04-04 F. Voisin , G. Rowell , M. G. Burton , A. Walsh , Y. Fukui , F. Aharonian

We have obtained high resolution mid-infrared images of the high mass protostar NGC 7538 IRS 1 using Michelle on Gemini North and find that the circumstellar dust associated with this source is extended on both large and small scales. The…

Astrophysics · Physics 2009-11-13 James M. De Buizer , Vincent Minier

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

This paper presents new near-infrared observations of the planetary nebula NGC 2346. The data include a broad K-band image, an image in the H2 vibrationally excited 1-0S(1) line and K band slit spectra at three positions in the nebula. In…

Astrophysics · Physics 2007-05-23 B. Vicini , A. Natta , A. Marconi , L. Testi , D. Hollenbach , B. T. Draine

Context. The high energies of protostellar jets, implied by recent observations of X-rays from such flows, came very much as a surprise. Inferred shock velocities are considerably higher than what was previously known, hence putting even…

Astrophysics · Physics 2009-11-11 R. Liseau

Mid-IR observations of planetary nebulae (PNe) have revealed diffuse emission associated to their main nebular shells and outer envelopes or haloes. The interpretation of this emission is uncertain because the broad-band mid-IR images may…

Astrophysics of Galaxies · Physics 2016-11-26 R. A. Marquez-Lugo , G. Ramos-Larios , M. A. Guerrero , R. Vazquez

We present Spitzer IRAC and IRS observations of the dark cloud L1287. The mid-infrared (MIR) IRAC images show deeply embedded infrared sources in the vicinity of the FU Orionis objects RNO 1B and RNO 1C suggesting their association with a…

Astrophysics · Physics 2009-01-19 S. P. Quanz , Th. Henning , J. Bouwman , H. Linz , F. Lahuis

Protostellar outflows display wide-angle winds and collimated jets, the magnetocentrifugal launching of which enables accretion onto the protostar. The majority of the outflow mass is likely ejected or entrained molecular H$_2$, which can…

We have made multi-epoch VLBI observations of H2O maser emission in the massive star forming region IRAS 06061+2151 with the Japanese VLBI network (JVN) from 2005 May to 2007 October. The detected maser features are distributed within an…

HH 110 and HH 262 are two Herbig-Haro jets with rather peculiar, chaotic morphology. In the two cases, no source suitable to power the jet has been detected along the outflow, at optical or radio wavelengths. Both, previous data and…

We report continuum GMRT observations aimed to explore the behavior of the jet associated with IRAS 16547-4247 at very low frequencies (325 MHz and 610 MHz). The obtained maps reveal an elongated morphology in the SE-NW direction. In…

Solar and Stellar Astrophysics · Physics 2018-12-19 Josep M. Masqué , Solay Jeyakumar , Miguel A. Trinidad , Tatiana Rodríguez-Esnard , CH Ishwara-Chandra

We probe the interstellar medium towards the objects Circinus X-1, a low-mass X-ray binary with relativistic jets; and the highly energetic Westerlund 2 stellar cluster, which is located towards TeV gamma-ray emission and interesting arc-…

High Energy Astrophysical Phenomena · Physics 2014-04-15 J. Hawkes , G. Rowell , B. Dawson , F. Aharonian , M. Burton , Y. Fukui , N. Furukawa , T. Hayakawa , A. Kawamura , N. Maxted , E. de Õna-Wilhelmi , P. de Wilt , A. Walsh

Herbig-Haro (HH) flows exhibit a large variety of morphological and kinematical structures such as bow shocks, Mach disks, and deflection shocks. Both proper motion (PM) and radial velocity investigations are essential to understand the…

Solar and Stellar Astrophysics · Physics 2019-07-10 T. A. Movsessian , T. Yu. Magakian , A. N. Burenkov

We discuss wide-field near-IR imaging of the NGC1333, L1448, L1455 and B1 star forming regions in Perseus. The observations have been extracted from a much larger narrow-band imaging survey of the Taurus-Auriga-Perseus complex. These H2…

Astrophysics · Physics 2009-06-23 C. J. Davis , P. Scholz , P. Lucas , M. D. Smith , A. Adamson

We present a long-slit spectrum of the Herbig-Haro object HH 111, obtained with SITS on the Hubble Space Telescope. This spectrum has a spectral resolution of approx. 50 km/s, so it gives a good picture of the kinematical properties of the…

One of the best-studied jets from all young stellar objects is the jet of DG Tau, which we imaged in the FUV with HST for the first time. These high spatial resolution images were obtained with long-pass filters and allow us to construct…

Solar and Stellar Astrophysics · Physics 2015-06-16 P. C. Schneider , J. Eisloeffel , M. Guedel , H. M. Guenther , G. Herczeg , J. Robrade , J. H. M. M. Schmitt