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Astronomy and Astrophysics, ISSN 0004-6361, 03/2005, Volume 431, Issue 3, pp. 905 - 924
We use archival Hubble Space Telescope observations of broad-band images from the ultraviolet (F255W-filter) through the near infrared (NICMOS F160W-filter) to... 
Galaxies: star clusters | Galaxies: individual: M 51
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 12/2019, Volume 633, p. A17
The grand-design spiral galaxy M 51 was observed at 40 pc resolution in CO(1-0) by the PAWS project. A large number of molecular clouds were identified and we... 
stars: formation | ISM: molecules | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | ISM: clouds | galaxies: individual: M 51 | galaxies: spiral
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 10/2005, Volume 441, Issue 3, pp. 949 - 960
In this work we concentrate on the evolution of the cluster population of the interacting galaxy M 51 (NGC 5194), more precisely the timescale of cluster... 
Galaxies: spiral | Galaxies: star clusters | Galaxies: individual: M 51 | METALLICITIES | TIME-SCALES | galaxies : spiral | M51 | galaxies : individual : M 51 | INTERACTING GALAXIES | PARAMETERS | galaxies : star clusters | DYNAMICAL MASS | CLOUDS | ASTRONOMY & ASTROPHYSICS | PHOTOMETRIC EVOLUTION | STELLAR POPULATIONS | GLOBULAR-CLUSTERS
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2007, Volume 469, Issue 3, pp. 925 - 940
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 08/2016, Volume 592, p. A123
A&A 592, A123 (2016) Cosmic ray electrons (CREs) are a crucial part of the ISM and are observed via synchrotron emission. While much modelling has been carried... 
Polarization | Galaxies: magnetic fields | Radio continuum: galaxies | Galaxies: individual: M 51 | Cosmic rays | Galaxies: ISM | Physics - Astrophysics of Galaxies
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 08/2018, Volume 478, Issue 3, pp. 3825 - 3831
As part of a wider investigation of evolved massive stars in Galactic open clusters, we have spectroscopically identified three candidate classical Cepheids in... 
PARALLAXES | open clusters and associations: individual: Berkeley 55 | CATALOG | Galaxy: structure | open clusters and associations: individual: NGC 6603 | PHOTOMETRY | ASTRONOMY & ASTROPHYSICS | PERIOD | PARAMETERS | stars: variables: Cepheids | open clusters and associations: individual: Berkeley 51
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 06/2016, Volume 459, Issue 2, pp. 1440 - 1467
We observed the spiral galaxies M 51 and M 83 at 20 arscec spatial resolution with the bolometer array Aztronomical Thermal Emission Camera (AzTEC) on the JCMT... 
galaxies: individual: M 51, M 83 | NEARBY GALAXIES | MODELING CO EMISSION | CO-TO-H-2 CONVERSION FACTOR | INTERSTELLAR-MEDIUM | COLUMN DENSITY | STAR-FORMATION LAW | GIANT MOLECULAR CLOUDS | EARLY-TYPE GALAXIES | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | HERSCHEL REFERENCE SURVEY | GALACTIC-CENTER REGION | galaxies: spiral
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2008, Volume 487, Issue 3, pp. 937 - 949
Context. Whether or not there exists a physical upper mass limit for star clusters is as yet unclear. For small cluster samples the mass function may not be... 
Galaxies: star clusters | Galaxies: individual: M 51
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 10/2011, Volume 740, Issue 2, p. 79
We present the results of detailed monitoring of the radio emission from the Type Ic supernova SN 1994I from three days after optical discovery on 1994 March... 
GAMMA-RAY BURST | SPIRAL GALAXIES | 1998BW | galaxies: individual (NGC 5194 [M 51]) | supernovae: general | RAPID PRESUPERNOVA EVOLUTION | radio continuum: stars | PROGENITOR | supernovae: individual (SN 1994I) | ASTRONOMY & ASTROPHYSICS | stars: mass-loss | IBC SUPERNOVAE | CONSTRAINTS | MASS-LOSS | SPECTRA | REMNANTS
Journal Article
Publications of the Astronomical Society of Japan, ISSN 0004-6264, 04/2014, Volume 66, Issue 2, p. 36
We have investigated the dynamics of the molecular gas and the evolution of giant molecular associations (GMAs) in the spiral galaxy M 51 with the Nobeyama... 
DENSITY WAVE | STAR-FORMATION | M51 | INTERSTELLAR-MEDIUM | PATTERN SPEEDS | radio lines: galaxies | N-BODY MODEL | RADIO-CONTINUUM | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | NOBEYAMA 45-M TELESCOPE | galaxies: kinematics and dynamics | galaxies: spiral | STELLAR MASS | galaxies: individual (M 51)
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2017, Volume 603, p. A57
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 08/2015, Volume 580, p. A142
Journal Article