9 papers · 1 filter
The distribution of the ISM in the Milky Way A three-dimensional large-scale model
A. Misiriotis, E. M. Xilouris, J. Papamastorakis +2
We use the COBE/DIRBE (1.2, 2.2, 60, 100, 140, and 240 m) maps and the COBE/FIRAS spectra (for the wavelength range 100 - 1000 m) to constrain a model for the spatial distrib…
Is the Galactic submillimeter dust emissivity underestimated?
K. M. Dasyra, E. M. Xilouris, A. Misiriotis +1
We present detailed modeling of the spectral energy distribution (SED) of the spiral galaxies NGC 891, NGC 4013, and NGC 5907 in the far-infrared and submm wavelengths. The model t…
Can rotation curves reveal the opacity of spiral galaxies ?
Angelos Misiriotis
Long-slit optical spectra along the major axis of spiral galaxies constitute a main source of information concerning the kinematics of galaxies. In highly inclined spiral galaxies…
Modelling the dust content of spiral galaxies: More dust mass vs. enhanced dust grain emissivity
K. M. Dasyra, E. M. Xilouris, A. Misiriotis +1
We present detailed modelling of the spectral energy distribution (SED) of the spiral galaxies NGC 891, NGC 4013, and NGC 5907 in the far-infrared (FIR) and sub-millimeter (submm)…
Dust in a merging galaxy sequence: the SCUBA view
A. Georgakakis, E. M. Xilouris, A. Misiriotis +1
We investigate the cold and warm dust properties during galaxy interactions using a merging galaxy sample ordered into a chronological sequence from pre- to post-mergers. Our sampl…
Cold and warm dust along a merging galaxy sequence
E. M. Xilouris, A. E. Georgakakis, A. Misiriotis +1
We investigate the cold and warm dust properties during galaxy interactions using a merging galaxy sample ordered into a chronological sequence from pre- to post-mergers. Our sampl…