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20032025
most citedThe Solar Orbiter mission -- Science overview

1.1k citations

Showing 2016Show all

9 papers · 1 filter

astro-ph.GA201636 cited

The Dense Molecular Gas and Nuclear Activity in the ULIRG IRAS 13120-5453

G. C. Privon, S. Aalto, N. Falstad +12

We present new ALMA Band 7 ( GHz) observations of the dense gas tracers HCN, HCO, and CS in the local, single-nucleus, ultraluminous infrared galaxy IRAS 13120-5453. W…

astro-ph.GA2016164 cited

Molecular outflows in local ULIRGs: energetics from multi-transition OH analysis

E. González-Alfonso, J. Fischer, H. W. W. Spoon +11

We report on the energetics of molecular outflows in 14 local Ultraluminous Infrared Galaxies (ULIRGs) that show unambiguous outflow signatures (P-Cygni profiles or high-velocity a…

astro-ph.GA201624 cited

Inflowing gas onto a compact obscured nucleus in Arp 299A: Herschel spectroscopic studies of H2O and OH

N. Falstad, E. González-Alfonso, S. Aalto +1

Aims. We probe the physical conditions in the core of Arp 299A and try to put constraints to the nature of its nuclear power source. Methods. We used Herschel Space Observatory far…

hep-ex2016236 cited

Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Aab, P. Abreu +435

Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models with…

astro-ph.GA201633 cited

HERUS: A CO Atlas from SPIRE Spectroscopy of local ULIRGs

Chris Pearson, Dimitra Rigopoulou, Peter Hurley +10

We present the Herschel SPIRE Fourier Transform Spectroscopy (FTS) atlas for a complete flux limited sample of local Ultra-Luminous Infra-Red Galaxies as part of the HERschel ULIRG…

astro-ph.SR20169 cited

Redefining the boundaries of interplanetary coronal mass ejections from observations at the ecliptic plane

C. Cid, J. Palacios, E. Saiz +1

On 2015 January 6-7, an interplanetary coronal mass ejection (ICME) was observed at L1. This event, which can be associated with a weak and slow coronal mass ejection, allows us to…