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We present Chandra observations of a small sample of nearby classical double radio galaxies which have more than one radio hotspot in at least one of their lobes. The X-ray emission from the hotspots of these comparatively low-power objects…

Astrophysics · Physics 2009-11-13 M. J. Hardcastle , J. H. Croston , R. P. Kraft

We report high spectral resolution (R=20,000) measurements of the H2 1-0 S(1) line in Herbig-Haro Objects 38, 46/47, and 120. The long-slit spectra reveal complex velocity structure with evidence for bow-shock structures as well as prompt…

Astrophysics · Physics 2009-11-07 Richard D. Schwartz , Thomas P. Greene

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

Radio emission from protostellar jets is usually dominated by free-free emission from thermal electrons. However, in some cases, it has been proposed that non-thermal emission could also be present. This additional contribution from…

Images made with the VLBA have resolved the region in a nearby radio galaxy, Pictor A, where the relativistic jet that originates at the nucleus terminates in an interaction with the intergalactic medium, a so-called radio galaxy hot spot.…

Astrophysics · Physics 2009-11-13 S. J. Tingay , E. Lenc , G. Brunetti , M. Bondi

We present observations of continuum emission in the MIR to mm wavelength range, complemented with ammonia observations, of the dense core ahead of the radio Herbig Haro object HH 80N, found in the GGD 27 region. The continuum emission in…

Using JWST near-infrared data of the inner Orion Nebula, \citet{Pearson_McCaughrean_2023} detected 40 binary systems they proposed to be Jupiter-Mass Binary Objects (JuMBOs) -- although their actual nature is still in debate. Only one of…

Earth and Planetary Astrophysics · Physics 2025-04-23 Luis F. Rodriguez , Laurent Loinard , Luis Zapata , Gisela N. Ortiz-Leon

We report Chandra X-ray Observatory and 1.4 GHz Australian Long Baseline Array (LBA) observations of the radio galaxy PKS 2153--69 and its environment. The Chandra image reveals a roughly spherical halo of hot gas extending out to 30 kpc…

Astrophysics · Physics 2009-11-10 A. J. Young , A. S. Wilson , S. J. Tingay , S. Heinz

We present new, high dynamic range VLA images of the inner jet of the closest radio galaxy, Centaurus A. Over a ten-year baseline we detect apparent sub-luminal motions (v ~ 0.5c) in the jet on scales of hundreds of pc. The inferred speeds…

Astrophysics · Physics 2008-11-26 M. J. Hardcastle , D. M. Worrall , R. P. Kraft , W. R. Forman , C. Jones , S. S. Murray

(abridged) The HH 80/81/80N jet extends from the HH 80 object to the recently discovered Source 34 and has a total projected jet size of 10.3 pc, constituting the largest collimated radio-jet system known so far. It is powered by IRAS…

The recent detection of X-ray emission from HH 2 and HH 154 with the Chandra and XMM-Newton satellites (respectively) have opened up an interesting, new observational possibility in the field of Herbig-Haro objects. In order to be able to…

Astrophysics · Physics 2009-11-07 A. C. Raga , A. Noriega-Crespo , P. F. Velazquez

Context. A molecular survey recently performed ahead of HH~2 supports the idea that the observed molecular enhancement is due to UV radiation from the HH object. Aims. The aim of the present work is to determine whether all HH objects with…

Astrophysics · Physics 2009-11-11 S. Viti , J. M. Girart , J. Hatchell

We report the discovery of spatially-extended, non-thermal-like emission components in Chandra X-ray spectra for five of a sample of seven massive, merging galaxy clusters with powerful radio halos. The emission components can be fitted by…

Astrophysics · Physics 2015-05-13 E. T. Million , S. W. Allen

Protostellar jets are one of the primary signposts of star formation. A handful of protostellar objects exhibit radio emission from ionized jets, of which a few display negative spectral indices, indicating the presence of synchrotron…

Astrophysics of Galaxies · Physics 2023-06-28 Sreelekshmi Mohan , Sarita Vig , Samir Mandal

We have observed 28 sources selected from the 1Jy sample of BL Lac objects (Stickel et al. 1991) with the Very Large Array (VLA) in A, B and D configurations at 1.36, 1.66 and 4.85 GHz, and/or with the Westerbork Synthesis Radio Telescope…

Astrophysics · Physics 2009-10-31 P. Cassaro , C. Stanghellini , M. Bondi , D. Dallacasa , R. Della Ceca , R. A. Zappala`

The giant Herbig-Haro object 222 extends over $\sim$6$'$ in the plane of the sky, with a bow shock morphology. The identification of its exciting source has remained uncertain over the years. A non-thermal radio source located at the core…

Solar and Stellar Astrophysics · Physics 2016-10-12 L. F. Rodriguez , J. O. Yam , C. Carrasco-Gonzalez , G. Anglada , A. Trejo

We present the first results from a recently concluded study of GRBs at $z\gtrsim5$ with the Karl G. Jansky Very Large Array (VLA). Spanning $1$ to $85.5$ GHz and 7 epochs from 1.5 to 82.3 d, our observations of GRB 140311A are the most…

High Energy Astrophysical Phenomena · Physics 2018-06-06 Tanmoy Laskar , Edo Berger , Ryan Chornock , Raffaella Margutti , Wen-fai Fong , Ashley Zauderer

We present a detailed analysis of Spitzer-IRAC images obtained toward six Herbig-Haro objects (HH 54/211/212, L 1157/1448, BHR 71). Our analysis includes: (1) comparisons in morphology between the four IRAC bands (3.6, 4.5, 5.8 and 8.0 um),…

Solar and Stellar Astrophysics · Physics 2015-05-19 Michihiro Takami , Jennifer L. Karr , Haegon Koh , How-Huan Chen , Hsu-Tai Lee

Hubble Space Telescope images obtained in 2018 are combined with archival HST data taken in 1995 to detect changes and measure proper motions in the HH 80/81 shock complex which is powered by the fastest known jet driven by a forming star,…

Astrophysics of Galaxies · Physics 2023-08-29 John Bally , Bo Reipurth

We present high-frequency, full-polarisation Jansky Very Large Array (VLA) radio data at X-band of the radio relic: MACS J0717.5+3745. Radio relics trace shock waves in the intracluster medium (ICM) produced during mergers. Understanding…

High Energy Astrophysical Phenomena · Physics 2025-11-10 A. Pasetto , O. Vilchis , A. Bonafede , E. F. Jiménez-Andrade , K. Rajpurohit , E. Murphy
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