Biblio

Found 7 results

Filters: Keyword is galaxies: ISM [Clear All Filters]

2015

The Influence of Supernova Remnants on the Interstellar Medium in the Large Magellanic Cloud Seen at 20-600 {$μ$}m Wavelengths, Lakićević, M., van Loon J. T., Meixner M., Gordon K., Bot C., Roman-Duval J., Babler B., Bolatto A., Engelbracht C., Filipović M., et al. , \apj, jan, Volume 799, p.50, (2015)

2014

The dust masses of powerful radio galaxies: clues to the triggering of their activity, Tadhunter, C., Dicken D., Morganti R., Konyves V., Ysard N., Nesvadba N., and C. Almeida Ramos , \mnras, Volume 445, p.L51-L55, (2014)

2012

The dust energy balance in the edge-on spiral galaxy NGC 4565, De Looze, I., Baes M., Bendo G. J., Ciesla L., Cortese L., de Geyter G., Groves B., Boquien M., Boselli A., Brondeel L., et al. , \mnras, dec, Volume 427, p.2797-2811, (2012)

2011

Efficient Three-dimensional NLTE Dust Radiative Transfer with SKIRT, Baes, M., Verstappen J., De Looze I., Fritz J., Saftly W., E. Pérez Vidal, Stalevski M., and Valcke S. , \apjs, oct, Volume 196, p.22, (2011)

Planck early results. XVII. Origin of the submillimetre excess dust emission in the Magellanic Clouds, Collaboration, Planck, Ade P. A. R., Aghanim N., Arnaud M., Ashdown M., Aumont J., Baccigalupi C., Balbi A., Banday A. J., Barreiro R. B., et al. , \aap, dec, Volume 536, p.A17, (2011)

Probing the dust properties of galaxies up to submillimetre wavelengths. II. Dust-to-gas mass ratio trends with metallicity and the submm excess in dwarf galaxies, Galametz, M., Madden S. C., Galliano F., Hony S., Bendo G. J., and Sauvage M. , \aap, aug, Volume 532, p.A56, (2011)

2010

Dust temperature tracing the ISRF intensity in the Galaxy, Bernard, J.-P., Paradis D., Marshall D. J., Montier L., Lagache G., Paladini R., Veneziani M., Brunt C. M., Mottram J. C., Martin P., et al. , \aap, jul, Volume 518, p.L88, (2010)