activity
20162024
most citedSubmillimeter H2O and H2O+ emission in lensed ultra- and hyper-luminous infrared galaxies at z ~ 2-4

67 citations · 235 across the 19 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

19 papers · 1 filter

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

A dusty proto-cluster surrounding the binary galaxy HerBS-70 at

Tom J. L. C. Bakx, S. Berta, H. Dannerbauer +38

We report on deep SCUBA-2 observations at 850m and NOEMA spectroscopic measurements at 2 mm of the environment surrounding the luminous, massive ($M_{*} \approx 2 \times 10^{11}…

astro-ph.GA20245 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.GA2024

Dust and Cold Gas Properties of Starburst HyLIRG-Quasars at

Feng-Yuan Liu, Y. Sophia Dai, Alain Omont +7

Some high-z active galactic nuclei (AGNs) are found to reside in extreme star-forming galaxies, such as hyper-luminous infrared galaxies (HyLIRGs), with AGN-removed o…

astro-ph.GA2023

The first ground-based detection of the 752 GHz water line in local ultra-luminous infrared galaxies using APEX-SEPIA

Daysi Quinatoa, Chentao Yang, Edo Ibar +10

We report the first ground-based detection of the water line p-H2O (211-202) at 752.033 GHz in three z < 0.08 ultra-luminous infrared galaxies (ULIRGs): IRAS 06035-7102, IRAS 17207…