activity
20082025
most citedALMA Observations of Warm Dense Gas in NGC 1614 --- Breaking of Star Formation Law in the Central kpc

67 citations · 174 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2025

Resolving the molecular gas emission of the z~2.5-2.8 starburst galaxies SPT0125-47 and SPT 2134-50

K. Kade, M. Bredberg, K. Knudsen +4

The comoving cosmic star formation rate density peaks at z~2-3, with dusty star-forming galaxies being significant contributors to this peak. These galaxies are characterized by th…

astro-ph.GA2025

High resolution ALMA observations of HS in LIRGS (Dense gas and shocks in outflows and CNDs)

M. T. Sato, S. Aalto, S. König +14

Molecular gas plays a critical role in regulating star formation and nuclear activity in galaxies. Sulphur bearing molecules, such as H2S, are sensitive to the physical and chemica…

astro-ph.GA2025

Searching for Compact Obscured Nuclei in Compton Thick AGN

Makoto A. Johnstone, George C. Privon, Loreto Barcos-Munoz +16

Compact Obscured Nuclei (CONs) are heavily obscured infrared cores that have been found in local (ultra)luminous infrared galaxies (U/LIRGs). They show bright emission from vibrati…

astro-ph.HE2025★ 8 cited

Millimeter emission from supermassive black hole coronae

S. del Palacio, C. Yang, S. Aalto +28

Active Galactic Nuclei (AGN) host accreting supermassive black holes (SMBHs). The accretion can lead to the formation of a hot, X-ray emitting corona close to the SMBH capable of a…

astro-ph.GA2025★ 8 cited

On unveiling Buried Nuclei with JWST: a technique for hunting the most obscured galaxy nuclei from local to high redshift

I. García-Bernete, F. R. Donnan, D. Rigopoulou +12

We analyze JWST NIRSpec+MIRI/MRS observations of the infrared (IR) Polycyclic Aromatic Hydrocarbon (PAH) features in the central regions (0.26'' at 6 micron; 50-440 pc…

astro-ph.GA2024

The fountain of the luminous infrared galaxy Zw049.057 as traced by its OH megamaser

Boy Lankhaar, Susanne Aalto, Clare Wethers +15

High resolution (0."037-0."13 [10-35 pc]) e-MERLIN ( cm) and (0."024 [6.5 pc]) ALMA ( mm) observations have been used to image OH (hydroxyl) and HCO (formald…

astro-ph.GA2024★ 5 cited

A spectacular galactic scale magnetohydrodynamic powered wind in ESO 320-G030

M. D. Gorski, S. Aalto, S. König +23

How galaxies regulate nuclear growth through gas accretion by supermassive black holes (SMBHs) is one of the most fundamental questions in galaxy evolution. One potential way to re…

astro-ph.GA2024

Double, double, toil, and trouble: The tails, bubbles, and knots of the local compact obscured nucleus galaxy NGC4418

C. F. Wethers, S. Aalto, G. C. Privon +20

Compact obscured nuclei (CONs) are an extremely obscured (N >10 cm) class of galaxy nuclei thought to exist in 20-40 per cent of nearby (ultra-)luminous infrar…

astro-ph.GA2023

Probing the interstellar medium of the quasar BRI0952-0115, an analysis of [CII], [CI], CO, OH, and H2O

K. Kade, K. K. Knudsen, A. Bewketu Belete +4

The extent of the effect of active galactic nuclei (AGN) on their host galaxies at high-redshift is not apparent and studying this effect in the distant universe is a difficult pro…

astro-ph.GA2022

A technique to select the most obscured galaxy nuclei

I. García-Bernete, D. Rigopoulou, S. Aalto +5

Compact obscured nuclei (CONs) are mainly found in local U/LIRGs. In the local Universe, these sources are generally selected through the detection of the HCN-vib (3-2) emission li…

astro-ph.GA2022★ 7 cited

APEX and NOEMA observations of HS in nearby luminous galaxies and the ULIRG Mrk~231 -- Is there a relation between dense gas properties and molecular outflows?

M. T. Sato, S. Aalto, K. Kohno +6

In order to understand the evolution and feedback of Active Galactic Nuclei (AGN) and star formation it is important to use molecular lines as probes of physical conditions and che…

astro-ph.GA2021★ 12 cited

Discovery of Methanimine Megamasers Toward Compact Obscured Galaxy Nuclei

Mark Gorski, Susanne Aalto, Jeffrey Mangum +8

We present the first search for the 5.29 GHz methanimine() transition toward a sample of galaxy nuclei. We target seven galaxies that host Compact…

astro-ph.GA2020★ 10 cited

VV 655 and NGC 4418: Implications of an interaction for the evolution of a LIRG

Erin Boettcher, John S. Gallagher, Youichi Ohyama +6

VV 655, a dwarf irregular galaxy with HI tidal debris, is a companion to the lenticular luminous infrared galaxy (LIRG) NGC 4418. NGC 4418 stands out among nearby LIRGs due to its…

astro-ph.GA2018★ 18 cited

Molecular gas in the northern nucleus of Mrk273: Physical and chemical properties of the disk and its outflow

R. Aladro, S. König, S. Aalto +12

Aiming to characterise the properties of the molecular gas in the ultraluminous infrared galaxy Mrk273 and its outflow, we used the NOEMA interferometer to image the dense gas mole…

astro-ph.GA2016★ 32 cited

Deep ALMA imaging of the merger NGC1614 - Is CO tracing a massive inflow of non-starforming gas?

S. König, S. Aalto, S. Muller +4

Observations of the molecular gas over scales of 0.5 to several kpc provide crucial information on how gas moves through galaxies, especially in mergers and interacting systems, wh…

astro-ph.GA2014★ 67 cited

ALMA Observations of Warm Dense Gas in NGC 1614 --- Breaking of Star Formation Law in the Central kpc

C. K. Xu, C. Cao, N. Lu +20

We present ALMA Cycle-0 observations of the CO (6-5) line emission and of the 435um dust continuum emission in the central kpc of NGC 1614, a local luminous infrared galaxy (LIRG)…

astro-ph2008★ 5 cited

Coordinated mm/sub-mm observations of Sagittarius A* in May 2007

D. Kunneriath, A. Eckart, S. Vogel +26

At the center of the Milky Way, with a distance of ~8 kpc, the compact source Sagittarius A* (SgrA*) can be associated with a super massive black hole of ~4x10^6 solar masses. SgrA…

astro-ph2008★ 2 cited

High-frequency VLBI observations of SgrA* during a multi-frequency campaign in May 2007

R. -S. Lu, T. P. Krichbaum, A. Eckart +5

In May 2007 the compact radio source Sgr A* was observed in a global multi-frequency monitoring campaign, from radio to X-ray bands. Here we present and discuss first and prelimina…