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NGC 5128 (Centaurus A) is one of the best example to study AGN-feedback in the local Universe. At 13.5 kpc from the galaxy, optical filaments with recent star formation are lying along the radio-jet direction. We used the Atacama Pathfinder…

Astrophysics of Galaxies · Physics 2016-11-09 Quentin Salomé , Philippe Salomé , Françoise Combes , Stephen Hamer

New BeppoSAX observations of the nearby archetypical starburst galaxies (SBGs) NGC253 and M82 are presented. The main observational result is the unambiguous evidence that the hard (2-10 keV) component is (mostly) produced in both galaxies…

We present a detailed analysis of J154506, a strongly lensed submillimeter galaxy behind the Lupus-I molecular cloud, and characterisation of its physical properties using a combination of new and archival data, including VLT/MUSE and FORS2…

We present Gemini-S/GMOS-IFU optical spectroscopy of four regions near the centre of the nearby (3.8 Mpc) dwarf starburst galaxy NGC 5253. This galaxy is famous for hosting a radio supernebula containing two deeply embedded massive super…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 M. S. Westmoquette , B. James , A. Monreal-Ibero , J. R. Walsh

We present high-spatial-resolution ($\sim 0\farcs2$, or $\sim$3\,pc) CO(2--1) observations of the nearest young starburst dwarf galaxy, NGC\,5253, taken with the Atacama Large Millimeter/submillimeter Array. We have identified 118 molecular…

Astrophysics of Galaxies · Physics 2018-10-10 Rie E. Miura , Daniel Espada , Akihiko Hirota , Kouichiro Nakanishi , George J. Bendo , Hajime Sugai

Magnetic fields are a good tracer for gas compression by shock waves, which can be caused by interaction of star-formation driven outflows from individual star formation sites as described in the chimney model. We study the magnetic field…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Volker Heesen , Rainer Beck , Marita Krause , Ralf-Jürgen Dettmar

We report on the Ka-band (26-40 GHz) emission properties for 10 star-forming regions in the nearby galaxy NGC 6946. From a radio spectral decomposition, we find that the 33 GHz flux densities are typically dominated by thermal (free-free)…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 E. J. Murphy , G. Helou , J. J. Condon , E. Schinnerer , J. L. Turner , R. Beck , B. S. Mason , R. -R. Chary , L. Armus

Combined Spitzer, Chandra, XMM-Newton, and VLA observations of the giant radio galaxy NGC 1316 (Fornax A) show a radio jet and X-ray cavities from AGN outbursts likely triggered by a merger with a late-type galaxy at least 0.4 Gyr ago. We…

Astrophysics of Galaxies · Physics 2015-05-19 Lauranne Lanz , Christine Jones , William R. Forman , Matthew L. N. Ashby , Ralph Kraft , Ryan C. Hickox

We used the NSF Jansky Very Large Array at a frequency $\nu =$ 22\,GHz to study the nearest billion-solar-mass black hole, in the early-type galaxy NGC\,3115 at a distance of 9.7\,Mpc. We localize a faint continuum nucleus, with flux…

Astrophysics of Galaxies · Physics 2025-08-12 J. M. Wrobel , D. W. Pesce , K. E. Nyland

We measure the extent of 100 micron galactic emission in two independent galaxy samples using the IRAS 100 micron Sky Survey images and constrain the distribution of dust at large ($\ltsim$30 kpc) radii. The first sample consists of 90…

Astrophysics · Physics 2009-10-30 Amy E. Nelson , Dennis Zaritsky , Roc M. Cutri

We present the results from a 42 ks \chandra ACIS observation of the galaxy cluster A478. This cluster is generally considered to be highly relaxed. The \chandra image reveals, for the first time, X-ray cavities in the hot gas within the…

Astrophysics · Physics 2009-09-17 M. Sun , C. Jones , S. S. Murray , S. W. Allen , A. C. Fabian , A. C. Edge

We use the radiation transfer simulation of Xilouris et al. (1999) to constrain the quantity of dust in three nearby spiral galaxies (NGC 4013, NGC 5907 and NGC 4565). The predicted visual optical depth from the model is compared with the…

Astrophysics · Physics 2009-11-10 P. B. Alton , E. M. Xilouris , A. Misiriotis , K. M. Dasyra , M. Dumke

We present the first maps of NGC 3044 and NGC 4157 at $\lambda\,450 \mu$m and $\lambda\,850 \mu$m from the JCMT as well as the first maps at 617 MHz from the GMRT. High latitude emission has been detected in both the radio continuum and…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 Judith A. Irwin , Rupinder S. Brar , D. J. Saikia , Richard N. Henriksen

Observations using the 7 mm receiver system on the Australia Telescope Compact Array have revealed large reservoirs of molecular gas in two high-redshift radio galaxies: HATLAS J090426.9+015448 (z = 2.37) and HATLAS J140930.4+003803 (z =…

Aims: Using XMM-Newton data, we have aimed to study the nuclear outflow of the nearby starburst galaxy NGC 253 in X-rays with respect to its morphology and to spectral variations along the outflow. Methods: We analysed XMM-Newton RGS…

Astrophysics · Physics 2009-11-11 M. Bauer , W. Pietsch , G. Trinchieri , D. Breitschwerdt , M. Ehle , A. Read

Three nearby galaxies which have abnormally high infrared to radio continuum ratios, NGC 1377, IC 1953 and NGC 4491, are investigated with a view to understanding the physical origin of their peculiarity. We review the existing data and…

Astrophysics · Physics 2009-11-07 H. Roussel , G. Helou , R. Beck , J. J. Condon , A. Bosma , K. Matthews , T. H. Jarrett

[abridged] We report on Suzaku observations of selected regions within the Southern giant lobe of the radio galaxy Centaurus A. We focus on distinct X-ray features likely associated with fine radio structure of the lobe. We find that the…

The VLBA and the VLA have been used to image the continuum radio emission from Mrk 231, a Seyfert 1 galaxy and the brightest infrared galaxy in the local universe. The smallest scales reveal a double source less than 2 pc in extent. The…

Astrophysics · Physics 2009-10-31 J. S. Ulvestad , J. M. Wrobel , C. L. Carilli

We report the detection of sub-mm emission from dust at 850 microns and of the 12CO J=4-3 line in the two distant powerful radio galaxies 4C 60.07 (z=3.79) and 6C 1909+722 (z=3.53). In the case of 4C 60.07 the dust emission is also detected…

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