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How does metallicity affect the gas and dust properties of galaxies?
Suzanne C. Madden, Diane Cormier and Aurélie Rémy-Ruyer Proceedings of the International Astronomical Union 11(S315) 191 (2015) https://doi.org/10.1017/S1743921316007493
Linking dust emission to fundamental properties in galaxies: the low-metallicity picture
Herschel-ATLAS: the surprising diversity of dust-selected galaxies in the local submillimetre Universe
C. J. R. Clark, L. Dunne, H. L. Gomez, et al. Monthly Notices of the Royal Astronomical Society 452(1) 397 (2015) https://doi.org/10.1093/mnras/stv1276
MEASURING STAR FORMATION RATES AND FAR-INFRARED COLORS OF HIGH-REDSHIFT GALAXIES USING THE CO(7–6) AND [N II] 205
μ
m LINES
Probing the interstellar medium of NGC 1569 with Herschel★
S. Lianou, P. Barmby, A. Rémy-Ruyer, et al. Monthly Notices of the Royal Astronomical Society 445(1) 1003 (2014) https://doi.org/10.1093/mnras/stu1770
DUST AND GAS IN THE MAGELLANIC CLOUDS FROM THE HERITAGEHERSCHELKEY PROJECT. I. DUST PROPERTIES AND INSIGHTS INTO THE ORIGIN OF THE SUBMILLIMETER EXCESS EMISSION
Dissecting the origin of the submillimetre emission in nearby galaxies with Herschel and LABOCA
M. Galametz, M. Albrecht, R. Kennicutt, et al. Monthly Notices of the Royal Astronomical Society 439(3) 2542 (2014) https://doi.org/10.1093/mnras/stu113
ALMA observations of cool dust in a low-metallicity starburst, SBS 0335−052
Constraining dust formation in high-redshift young galaxies
Hiroyuki Hirashita, Andrea Ferrara, Pratika Dayal and Masami Ouchi Monthly Notices of the Royal Astronomical Society 443(2) 1704 (2014) https://doi.org/10.1093/mnras/stu1290
Dust origin in late-type dwarf galaxies: ISM growth vs. type II supernovae
Herschel/PACS observations of the host galaxy of GRB 031203
M. Symeonidis, S. R. Oates, M. de Pasquale, M. J. Page, K. Wiersema, R. Starling, P. Schady, N. Seymour and B. O'Halloran Monthly Notices of the Royal Astronomical Society: Letters 443(1) L124 (2014) https://doi.org/10.1093/mnrasl/slu090
The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types