about
Gone with the heat: a fundamental constraint on the imaging of dust and molecular gas in the early UniverseThe Herschel Virgo Cluster Survey VI. The far-infrared view of M 87The Herschel Virgo Cluster Survey III. A constraint on dust grain lifetime in early-type galaxiesTracing the molecular gas in distant submillimetre galaxies via CO(1-0) imaging with the Expanded Very Large ArrayDust emission in early-type galaxies: The mid-infrared viewMeasuring star formation with resolved observations: the test case of M 33Variation in the dust emissivity index across M 33 with Herschel and Spitzer (HerM 33es)Spectral energy distributions of H ii regions in M 33 (HerM33es)Cool and warm dust emission from M 33 (HerM33es)Dust and gas power spectrum in M 33 (HERM33ES)Dust heating sources in galaxies: the case of M33 (HERM33ES)Molecular and atomic gas in the Local Group galaxy M 33100 μm and 160 μm emission as resolved star-formation rate estimators in M 33 (HERM33ES)Cool gas and dust in M 33: Results from the HERschel M 33 Extended Survey (HERM33ES)PACS and SPIRE photometer maps of M 33: First results of the HERschel M 33 Extended Survey (HERM33ES)Properties of compact 250 μm emission and H II regions in M 33 (HERM33ES)The Herschel Virgo Cluster Survey XIII. Dust in early-type galaxiesThe Herschel Fornax Cluster Survey – I. The bright galaxy sampleThe Herschel Virgo Cluster Survey – XII. FIR properties of optically selected Virgo cluster galaxiesThe Herschel reference survey: dust in early-type galaxies and across the Hubble sequenceDust Content of Virgo Star-Forming Dwarf GalaxiesDust in Cluster Dwarf Elliptical GalaxiesThe GALEX Ultraviolet Virgo Cluster Survey (GUViCS)The far-infrared view of M87 as seen by the Herschel Space ObservatoryFIR colours and SEDs of nearby galaxies observed with HerschelThe Herschel Virgo Cluster Survey II. Truncated dust disks in H I-deficient spiralsThe Herschel Virgo Cluster Survey IV. Resolved dust analysis of spiral galaxiesThe Herschel Virgo Cluster Survey I. Luminosity functionThe Herschel Virgo Cluster Survey VII. Dust in cluster dwarf elliptical galaxiesThe Herschel Virgo Cluster Survey V. Star-forming dwarf galaxies – dust in metal-poor environmentsNELIOTA: First temperature measurement of lunar impact flashesThe physical properties ofSpitzer/IRS galaxies derived from their UV to 22μm spectral energy distributionNELIOTA: ESA's new NEO lunar impact monitoring project with the 1.2m telescope at the National Observatory of AthensConstraining the properties of AGN host galaxies with spectral energy distribution modellingThe Herschel comprehensive (U)LIRG emission survey (HERCULES): CO ladders, fine structure lines, and neutral gas coolingA mid-IR study of Hickson compact groupsBlack hole accretion and star formation as drivers of gas excitation and chemistry in Markarian 231Herschel observations of water vapour in Markarian 231Cold and warm dust along a merging galaxy sequenceRadial distribution of dust, stars, gas, and star-formation rate in DustPedia face-on galaxies
P50
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P50
description
Greek astrophysicist
@en
astrofísico griego
@es
astrophysicien grec
@fr
onderzoeker uit Griekenland
@nl
name
Manolis Xilouris
@ast
Manolis Xilouris
@en
Manolis Xilouris
@es
Manolis Xilouris
@fr
Manolis Xilouris
@ga
Manolis Xilouris
@nl
Manolis Xilouris
@sq
type
label
Manolis Xilouris
@ast
Manolis Xilouris
@en
Manolis Xilouris
@es
Manolis Xilouris
@fr
Manolis Xilouris
@ga
Manolis Xilouris
@nl
Manolis Xilouris
@sq
altLabel
E. M. Xilouris
@en
prefLabel
Manolis Xilouris
@ast
Manolis Xilouris
@en
Manolis Xilouris
@es
Manolis Xilouris
@fr
Manolis Xilouris
@ga
Manolis Xilouris
@nl
Manolis Xilouris
@sq