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Unveiling the inner morphology and gas kinematics of NGC 5135 with ALMA
G. Sabatini, C. Gruppioni, M. Massardi +5
The local Seyfert 2 galaxy NGC5135, thanks to its almost face-on appearance, a bulge overdensity of stars, the presence of a large-scale bar, an AGN and a Supernova Remnant, is an…
CO excitation in the Seyfert galaxy NGC 34: stars, shock or AGN driven?
M. Mingozzi, L. Vallini, F. Pozzi +7
We present a detailed analysis of the X-ray and molecular gas emission in the nearby galaxy NGC 34, to constrain the properties of molecular gas, and assess whether, and to what ex…
Unbiased large spectroscopic surveys of galaxies selected by SPICA using dust bands
H. Kaneda, D. Ishihara, S. Oyabu +27
The mid-infrared (IR) range contains many spectral features associated with large molecules and dust grains such as polycyclic aromatic hydrocarbons (PAHs) and silicates. These are…
Tracing the evolution of dust obscured star-formation and accretion back to the reionisation epoch with SPICA
C. Gruppioni, L. Ciesla, E. Hatziminaoglou +35
Our current knowledge of star formation and accretion luminosity at high-redshift (z>3-4), as well as the possible connections between them, relies mostly on observations in the re…
Galaxy evolution studies with the SPace IR telescope for Cosmology and Astrophysics (SPICA): the power of IR spectroscopy
L. Spinoglio, A. Alonso-Herrero, L. Armus +65
IR spectroscopy in the range 12-230 micron with the SPace IR telescope for Cosmology and Astrophysics (SPICA) will reveal the physical processes that govern the formation and evolu…
SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust
J. A. Fernández-Ontiveros, L. Armus, M. Baes +33
The physical processes driving the chemical evolution of galaxies in the last cannot be understood without directly probing the dust-obscured phase of star-for…