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Browsing by Author "Anglés-Alcázar, D."
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Energy balance SED modelling can be effective at high redshifts regardless of UV-FIR offsets
Haskell, P.; Smith, D. J. B.; Cochrane, R. K.; Hayward, C. C.; Anglés-Alcázar, D. (2023-10-01)Recent works have suggested that energy balance spectral energy distribution (SED) fitting codes may be of limited use for studying high-redshift galaxies for which the observed ultraviolet and far-infrared emission are ... -
A Herschel study of YSO evolutionary stages and formation timelines in two fields of the Hi-GAL survey
Elia, D.; Schisano, E.; Molinari, S.; Robitaille, T.; Anglés-Alcázar, D.; Bally, J.; Battersby, C.; Benedettini, M.; Billot, N.; Calzoletti, L.; Di Giorgio, A. M.; Faustini, F.; Li, J. Z.; Martin, P.; Morgan, L.; Motte, F.; Mottram, J.C.; Natoli, P.; Olmi, L.; Paladini, R.; Piacentini, F.; Pestalozzi, M.; Pezzuto, S.; Polychroni, D.; Smith, M.; Strafella, F.; Stringfellow, G. S.; Testi, L.; Thompson, M.A.; Traficante, A.; Veneziani, M. (2010-05-11)We present a first study of the star-forming compact dust condensations revealed by Herschel in the two 2 \times 2 \degr Galactic Plane fields centered at [l;b] = [30\degr; 0 \degr] and [l;b] = [59\degr; 0 \degr], respectively, ... -
On the shape of the mass-function of dense clumps in the Hi-GAL fields . I : Spectral energy distribution determination and global properties of the mass-functions
Olmi, L.; Anglés-Alcázar, D.; Elia, D.; Molinari, S.; Montier, L.; Pestalozzi, M.; Pezzuto, S.; Polychroni, D.; Ristorcelli, I.; Rodon, J.; Schisano, E.; Smith, M.D.; Testi, L.; Thompson, M. (2013-03-01)Context. Stars form in dense, dusty clumps of molecular clouds, but little is known about their origin and evolution. In particular, the relationship between the mass distribution of these clumps (also known as the clump ... -
On the shape of the mass-function of dense clumps in the Hi-GAL fields II : Using Bayesian inference to study the clump mass function
Olmi, L.; Anglés-Alcázar, D.; Elia, D.; Molinari, S.; Pestalozzi, M.; Pezzuto, S.; Schisano, E.; Testi, L.; Thompson, M.A. (2014-04)Context. Stars form in dense, dusty clumps of molecular clouds, but little is known about their origin, their evolution, and their detailed physical properties. In particular, the relationship between the mass distribution ...