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A triple radio source recently detected in association with the luminous infrared source IRAS 16547-4247 has been studied with high angular resolution and high sensitivity with the Very Large Array at 3.6 and 2 cm. Our observations confirm…

Astrophysics · Physics 2009-11-10 L. F. Rodriguez , G. Garay , K. J. Brooks , D. Mardones

We report sensitive VLA 3.6 cm radio observations toward the head of the Cone nebula in NGC 2264, made in 2006. The purpose of these observations was to study a non-thermal radio jet recently discovered, that appears to emanate from the…

Astrophysics · Physics 2009-11-13 A. Trejo , Luis F. Rodriguez

We present recent Very Long Baseline Array (VLBA) 5 GHz radio observations of the nearby, luminous Seyfert 2 galaxy NGC 1068 for comparison to similar VLBA observations made on 1997 April 26. By cross-correlating the positions of emitting…

Astrophysics of Galaxies · Physics 2023-08-16 Travis C. Fischer , Megan C. Johnson , Nathan J. Secrest , D. Michael Crenshaw , Steven B. Kraemer

We present VLA 3.5 cm continuum observations of the Serpens cloud core. 22 radio continuum sources are detected. 16 out of the 22 cm sources are suggested to be associated with young stellar objects (Class 0, Class I, flat-spectrum, and…

Astrophysics · Physics 2008-11-26 C. Eiroa , J. M. Torrelles. S. Curiel , A. A. Djupvik

We report the discovery of an extremely curved jet in the radio-loud quasar PKS2136+141. Multi-frequency Very Long Baseline Array (VLBA) images show a bending jet making a turn-around of 210 degrees in the plane of the sky, which is, to our…

Recently, there has been an increased interest in the study of the generation of low-energy cosmic rays (CRs; < 1 TeV) in shocks situated on the surface of a protostar or along protostellar jets. These locally accelerated CRs offer an…

High Energy Astrophysical Phenomena · Physics 2021-06-02 Marco Padovani , Alexandre Marcowith , Daniele Galli , Leslie K. Hunt , Francesco Fontani

An increasing number of blazars have been reported to show jet wobbling (i.e., non-regular rotations of the structural position angle of their innermost jets in the plane of the sky with amplitudes between 20 deg. and 50 deg., and time…

Astrophysics · Physics 2008-03-25 I. Agudo

The head--tail (HT) morphology of radio galaxies is seen for a class of radio sources where the primary lobes are being bent in the intercluster weather due to strong interactions between the radio jets and their respective intracluster…

Astrophysics of Galaxies · Physics 2025-12-16 Tapan K. Sasmal , Soumen Bera , Sabyasachi Pal , Soumen Mondal

As the closest known active galactic nucleus, Centaurus A (Cen A) provides a rich environment for astrophysical exploration. It has been observed across wavelengths from radio to gamma rays, and indications of ongoing particle acceleration…

High Energy Astrophysical Phenomena · Physics 2025-04-04 Cainã de Oliveira , James H. Matthews , Vitor de Souza

Until recently, there have been few studies of the protostellar evolution of intermediate-mass (IM) stars, which may bridge the low- and high-mass regimes. This paper aims to investigate whether the properties of an IM protostar within the…

Astrophysics of Galaxies · Physics 2016-09-01 G. M. Brown , K. G. Johnston , M. G. Hoare , S. L. Lumsden

We present a ~100 ksec Chandra X-ray observation and new VLA radio data of the large scale, 300 kpc long X-ray jet in PKS1127-145, a radio loud quasar at redshift z=1.18. With this deep X-ray observation we now clearly discern the complex…

Bright features (`knots') in extragalactic jets are commonly associated with reheating of charged particles in regions with shocks or strong compression. We find a natural appearance of nozzles in simulations of toroidally magnetized jets,…

Astrophysics · Physics 2007-05-23 Maurice H. P. M. van Putten

I present 1.5- and 8.4-GHz observations with all configurations of the NRAO VLA of the wide-angle tail source 3C130. The source has a pair of relatively symmetrical, well-collimated inner jets, one of which terminates in a compact hot spot.…

Astrophysics · Physics 2009-10-30 M. J. Hardcastle

A multiwavelength analysis of star formation associated with the extended green object, G19.88-0.53 is presented in this paper. With multiple detected radio and millimetre components, G19.88-0.53 unveils as harbouring a protocluster rather…

We present high angular resolution VLA and BIMA observations of NH$_3$, HCO$^+$, HCN and SO molecular emission and 1.4, 3.5 and 7 mm continuum emission toward the exciting source of the HH~80-81 system. This object is one of the few massive…

Astrophysics · Physics 2012-08-27 Y. Gomez , L. F. Rodriguez , J. M. Girart , G. Garay , andJ. Marti

We present VLA and first-epoch VLBA observations that are part of a program to study the parsec-scale radio structure of a sample of fifteen high-energy-peaked BL Lacs (HBLs). The sample was chosen to span the range of logarithmic X-ray to…

Astrophysics · Physics 2009-11-07 T. A. Rector , D. C. Gabuzda , J. T. Stocke

HH 212 is a nearby (460 pc) protostellar jet discovered in H$_2$ powered by a Class 0 source, IRAS 05413-0104, in the L1630 cloud of Orion. It is highly collimated and symmetric with matched pairs of bow shocks on either side of the source.…

The study of Head Tail (HT) radio galaxies track the information of associated galaxy clusters. With the help of the VLA FIRST survey at 1.4 GHz, we detected 607 new HT radio sources, among them, 398 are Wide Angle Tail (WAT) and 216 are…

High Energy Astrophysical Phenomena · Physics 2021-03-30 Sabyasachi Pal , Shobha Kumari

The FRI/FRII dichotomy is a much debated issue in the astrophysics of extragalactic radio sources. Study of the properties of HYbrid MOrphology Radio Sources (HYMORS) may bring crucial information and lead to a step forward in understanding…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 Maciej Ceglowski , Marcin Gawronski , Magdalena Kunert-Bajraszewska

We employed the Very Large Array (VLA) of the National Radio Astronomy Observatory in C configuration to map 39 ultraluminous IRAS galaxies at 6~cm and 20~cm, at resolutions of ~ 4" and 15", respectively, and 24 sources at 6~cm with in the…

Astrophysics · Physics 2008-11-26 Thomas Crawford , Jon Marr , Bruce Partridge , Michael Strauss