61 citations · 245 across the 11 of their papers we have counts for
12 papers
Nuclear Millimeter Continuum Emission in Radio-Quiet Active Galactic Nuclei: an ALMA Spectral and Variability Study
Sophie M. Venselaar, Claudio Ricci, Yoshiyuki Inoue +8
Unresolved millimeter (mm) emission is observed in radio-quiet (RQ) Active Galactic Nuclei (AGN), but its physical origin remains debated. Self-absorbed synchrotron emission from t…
The PARADIGM Project II: Characterising Nuclear and Diffuse Radio Components in Local U/LIRGs
Geferson Lucatelli, Rob Beswick, Javier Moldón +14
Disentangling SF and AGN emission is essential for understanding galaxy evolution, yet remains challenging in merging systems where both processes are enhanced and spatially intert…
A consistent radio to sub-mm pc-scale study of the nucleus of NGC 1068
Isaac M. Mutie, Santiago del Palacio, Robert J. Beswick +5
The origin of radio emission in radio-quiet (RQ) AGN remains a long-standing mystery. We present a detailed study of the cm to sub-mm emission from the nucleus of the nearby protot…
The PARADIGM Project I: A Multiscale radio morphological analysis of local U/LIRGS
G. Lucatelli, R. Beswick, J. Moldon +12
Disentangling the radio flux contribution from star formation (SF) and active-galactic-nuclei (AGN) activity is a long-standing problem in extragalactic astronomy, since at frequen…
Radio jets in NGC 1068 with e-MERLIN and VLA: structure and morphology
Isaac M. Mutie, David Williams-Baldwin, Robert J. Beswick +7
We present new high-sensitivity e-MERLIN and VLA radio images of the prototypical Seyfert 2 galaxy NGC 1068 at 5, 10 and 21 GHz. We image the radio jet, from the compact components…
An atomic hydrogen bridge fueling NGC 4418 with gas from VV 655
E. Varenius, F. Costagliola, H. -R. Klöckner +4
The galaxy NGC 4418 harbours a compact ( pc) core with a very high bolometric luminosity (L). As most of the galaxy's energy output comes from this small…
The population of SNe/SNRs in the starburst galaxy Arp 220. A self-consistent analysis of 20 years of VLBI monitoring
E. Varenius, J. E. Conway, F. Batejat +6
The nearby ultra-luminous infrared galaxy (ULIRG) Arp 220 is an excellent laboratory for studies of extreme astrophysical environments. For 20 years, Very Long Baseline Interferome…
Subarcsecond international LOFAR radio images of Arp 220 at 150 MHz: A kpc-scale star forming disk surrounding nuclei with shocked outflows
E. Varenius, J. E. Conway, I. Martí-Vidal +16
We analyse new observations with the International Low Frequency Array (LOFAR) telescope, and archival data from the Multi-Element Radio Linked Interferometer Network (MERLIN) and…
Subarcsecond international LOFAR radio images of the M82 nucleus at 118 MHz and 154 MHz
E. Varenius, J. E. Conway, I. Martí-Vidal +25
The nuclear starburst in the nearby galaxy M82 provides an excellent laboratory for understanding the physics of star formation. This galaxy has been extensively observed in the pa…
The NGC 1614 Interacting Galaxy: Molecular Gas Feeding a "Ring of Fire"
S. König, S. Aalto, S. Muller +2
Minor mergers frequently occur between giant and gas-rich low mass galaxies and can provide significant amounts of interstellar matter to refuel star formation and power AGN in the…
Densitometry and Thermometry of Starburst Galaxies
Jeffrey G. Mangum, Jeremy Darling, Karl M. Menten +2
With a goal toward deriving the physical conditions in external galaxies, we present a survey of formaldehyde (H2CO) and ammonia (NH3) emission and absorption in a sample of starbu…
Star-formation in the central kpc of the starburst/LINER galaxy NGC1614
E. Olsson, S. Aalto, M. Thomasson +1
A high angular resolution, multi-wavelength study of the LINER galaxy NGC1614 has been carried out. OVRO CO 1-0 observations are presented together with extensive multi-frequency r…