activity
20112024
most citedStar cluster formation in the most extreme environments: Insights from the HiPEEC survey

79 citations · 632 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.GA2024★ 11 cited

CON-quest II. Spatially and spectrally resolved HCN/HCO+ line ratios in local luminous and ultraluminous infrared galaxies

Y. Nishimura, S. Aalto, M. D. Gorski +24

Nuclear regions of ultraluminous and luminous infrared galaxies (U/LIRGs) are powered by starbursts and/or active galactic nuclei (AGNs). These regions are often obscured by extrem…

astro-ph.GA2024

The ALCHEMI atlas: principal component analysis reveals starburst evolution in NGC 253

Nanase Harada, David S. Meier, Sergio Martín +24

Molecular lines are powerful diagnostics of the physical and chemical properties of the interstellar medium (ISM). These ISM properties, which affect future star formation, are exp…

astro-ph.GA2023

Large-Scale Features of the CON Galaxy NGC4418 with MUSE

C. F. Wethers, S. Aalto, G. C. Privon +6

Compact obscured nuclei (CONs) are relatively common in the centers of local (U)LIRGs, yet their nature remains unknown. Both AGN activity and extreme nuclear starbursts have been…

astro-ph.GA2023

5-12 pc resolution ALMA imaging of gas and dust in the obscured compact nucleus of IRAS 17578-0400

Chentao Yang, Susanne Aalto, Sabine König +7

We here present 0.02-0.04'' resolution ALMA observation of the compact obscured nucleus (CON) of IRAS17578-0400. A dusty torus within the nucleus, approximately 4 pc in radius, has…

astro-ph.GA2022★ 12 cited

The Opaque Heart of the Galaxy IC 860: Analogous Protostellar, Kinematics, Morphology, and Chemistry

M. D. Gorski, S. Aalto, S. König +7

Compact Obscured Nuclei (CONs) account for a significant fraction of the population of luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs). These galaxy nuclei are comp…

astro-ph.GA2020★ 18 cited

Planck's Dusty GEMS. VIII. Dense-gas reservoirs in the most active dusty starbursts at z~3

R. Canameras, N. P. H. Nesvadba, R. Kneissl +6

We present ALMA, NOEMA, and IRAM-30m/EMIR observations of the high-density tracer molecules HCN, HCO+, and HNC in three of the brightest lensed dusty star-forming galaxies at z~3-3…

astro-ph.GA2020★ 79 cited

Star cluster formation in the most extreme environments: Insights from the HiPEEC survey

A. Adamo, K. Hollyhead, M. Messa +14

We present the Hubble imaging Probe of Extreme Environments and Clusters (HiPEEC) survey. We fit HST NUV to NIR broadband and H fluxes, to derive star cluster ages, masses, exti…

astro-ph.GA2020★ 31 cited

ALMA resolves the remarkable molecular jet and rotating wind in the extremely radio-quiet galaxy NGC 1377

S. Aalto, N. Falstad, S. Muller +14

Submillimetre and millimetre observations are important in probing the properties of the molecular gas and dust around obscured active galactic nuclei (AGNs) and their feedback. Wi…

astro-ph.GA2019★ 34 cited

A spectral stacking analysis to search for faint outflow signatures in z~6 quasars

F. Stanley, J. B. Jolly, S. König +1

Outflows in quasars during the early epochs of galaxy evolution are an important part of the feedback mechanisms potentially affecting the evolution of the host galaxy. However, sy…

astro-ph.GA2019★ 56 cited

The hidden heart of the luminous infrared galaxy IC 860 I. A molecular inflow feeding opaque, extreme nuclear activity

S. Aalto, S. Muller, S. König +19

High-resolution (0."03 - 0."09) (9 - 26 pc)) ALMA (100 - 350 GHz (3 - 0.8 mm)) and VLA 45 GHz measurements have been used to image continuum and spectral line emission from the inn…

astro-ph.GA2019★ 37 cited

Hidden or missing outflows in highly obscured galaxy nuclei?

N. Falstad, F. Hallqvist, S. Aalto +19

Understanding the nuclear growth and feedback processes in galaxies requires investigating their often obscured central regions. One way to do this is to use (sub)millimeter line e…

astro-ph.GA2018★ 45 cited

Planck's Dusty GEMS. VII. Atomic carbon and molecular gas in dusty starburst galaxies at z=2 to 4

N. Nesvadba, R. Canameras, R. Kneissl +5

The bright [CI] 1-0 and [CI] 2-1 lines of atomic carbon are becoming more and more widely employed tracers of the cold neutral gas in high-redshift galaxies. Here we present observ…

astro-ph.GA2018★ 69 cited

Planck's dusty GEMS. VI. Multi-J CO excitation and interstellar medium conditions in dusty starburst galaxies at z=2-4

R. Canameras, C. Yang, N. P. H. Nesvadba +8

We present an extensive CO emission-line survey of the Planck's dusty GEMS, a small set of 11 strongly lensed dusty star-forming galaxies at z = 2-4 discovered with Planck and Hers…

astro-ph.GA2018★ 29 cited

Planck's dusty GEMS. V. Molecular wind and clump stability in a strongly lensed star-forming galaxy at z=2.2

R. Canameras, N. P. H. Nesvadba, M. Limousin +6

We report the discovery of a molecular wind signature from a massive intensely star-forming clump of a few Msun, in the strongly gravitationally lensed submillimeter galaxy…

astro-ph.GA2017★ 11 cited

Major impact from a minor merger - The extraordinary hot molecular gas flow in the Eye of the NGC 4194 Medusa galaxy

S. König, S. Aalto, S. Muller +6

Minor mergers are important processes contributing significantly to how galaxies evolve across the age of the Universe. Their impact on supermassive black hole growth and star form…

astro-ph.GA2017★ 19 cited

A hidden molecular outflow in the LIRG Zw 049.057

N. Falstad, S. Aalto, J. G. Mangum +8

Feedback in the form of mass outflows driven by star formation or active galactic nuclei is a key component of galaxy evolution. The luminous infrared galaxy Zw 049.057 harbours a…

astro-ph.GA2017★ 23 cited

Luminous, pc-scale CO 6-5 emission in the obscured nucleus of NGC1377

S. Aalto, S. Muller, F. Costagliola +13

High resolution submm observations are important in probing the morphology, column density and dynamics of obscured active galactic nuclei (AGNs). With high resolution (0.06 x 0.05…

astro-ph.GA2016★ 32 cited

Spatially resolved CO SLED of the Luminous Merger Remnant NGC 1614 with ALMA

Toshiki Saito, Daisuke Iono, Cong K. Xu +13

We present high-resolution (1".0) Atacama Large Millimeter/submillimeter Array (ALMA) observations of CO (1-0) and CO (2- 1) rotational transitions toward the nearby IR-luminous me…

astro-ph.GA2016★ 21 cited

Sub-arcsecond imaging of the water emission in Arp 220

S. König, S. Martín, S. Muller +14

Extragalactic observations of water emission can provide valuable insights into the excitation of the interstellar medium. In addition, extragalactic megamasers are powerful probes…

astro-ph.GA2016★ 61 cited

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…

astro-ph.GA2014★ 9 cited

Molecular tendrils feeding star formation in the Eye of the Medusa - The Medusa merger in high resolution 12CO 2-1 maps

S. König, S. Aalto, L. Lindroos +5

Studying molecular gas properties in merging galaxies gives us important clues to the onset and evolution of interaction-triggered starbursts. NGC4194 is particularly interesting t…

astro-ph.CO2013★ 27 cited

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…

astro-ph.CO2011★ 8 cited

A search for water maser emission in nearby low-luminosity QSO host galaxies

S. König, A. Eckart, C. Henkel +1

A sample of nearby galaxies hosting low-luminosity type 1 quasi-stellar objects (QSOs), previously studied in CO and HI emission lines, has been searched for maser emission. Using…