L
Luigi Spinoglio
Researcher at INAF
Publications - 223
Citations - 13873
Luigi Spinoglio is an academic researcher from INAF. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 61, co-authored 222 publications receiving 12904 citations.
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Journal ArticleDOI
Characterizing interstellar filaments with Herschel in IC 5146
Doris Arzoumanian,Ph. André,Pierre Didelon,Vera Könyves,Nicola Schneider,Alexander Men'shchikov,Thierry Sousbie,Annie Zavagno,Sylvain Bontemps,J. Di Francesco,Matthew Joseph Griffin,M. Hennemann,Tracey Hill,Jason M. Kirk,Peter G. Martin,Vincent Minier,Sergio Molinari,Frédérique Motte,Nicolas Peretto,Stefano Pezzuto,Luigi Spinoglio,Derek Ward-Thompson,Glenn J. White,Christine D. Wilson +23 more
TL;DR: In this paper, the results of the Herschel Gould Belt survey toward the IC 5146 molecular cloud were analyzed and a preliminary analysis of the filamentary structure in this region was presented.
Journal ArticleDOI
Characterizing interstellar filaments with Herschel in IC5146
Doris Arzoumanian,Ph. André,Pierre Didelon,Vera Konyves,Nicola Schneider,Alexander Men'shchikov,Thierry Sousbie,Annie Zavagno,Sylvain Bontemps,J. Di Francesco,Matthew Joseph Griffin,M. Hennemann,Tracey Hill,Jason M. Kirk,Pierrick Martin,Vincent Minier,Sergio Molinari,Frédérique Motte,Nicolas Peretto,Stefano Pezzuto,Luigi Spinoglio,Derek Ward-Thompson,G. J. White,Christine D. Wilson +23 more
TL;DR: In this paper, the results of the Herschel Gould Belt survey toward the IC5146 molecular cloud were analyzed and a preliminary analysis of the filamentary structure in this region was presented.
Journal ArticleDOI
Herschel view of the Taurus B211/3 filament and striations: evidence of filamentary growth?
P. Palmeirim,Ph. André,Jason M. Kirk,Derek Ward-Thompson,Doris Arzoumanian,Vera Könyves,Vera Könyves,Pierre Didelon,Nicola Schneider,Nicola Schneider,M. Benedettini,Sylvain Bontemps,J. Di Francesco,J. Di Francesco,Davide Elia,Matthew Joseph Griffin,M. Hennemann,Tracey Hill,Peter G. Martin,Alexander Men'shchikov,Sergio Molinari,Frédérique Motte,Q. Nguyen Luong,David John Nutter,Nicolas Peretto,Stefano Pezzuto,A. Roy,Kazi L.J. Rygl,Luigi Spinoglio,G. L. White,G. L. White +30 more
TL;DR: In this article, the results from the Herschel Gould Belt survey for the B211/L1495 region in the Taurus molecular cloud were presented, which revealed the structure of the dense, star-forming filament B211 with unprecedented detail, along with the presence of striations perpendicular to the filament.
Journal ArticleDOI
Herschel view of the Taurus B211/3 filament and striations: Evidence of filamentary growth?
P. Palmeirim,Ph. André,Jason M. Kirk,Derek Ward-Thompson,Doris Arzoumanian,Vera Konyves,Pierre Didelon,Nicola Schneider,M. Benedettini,Sylvain Bontemps,J. Di Francesco,Davide Elia,Matthew Joseph Griffin,M. Hennemann,Tracey Hill,Pierrick Martin,Alexander Men'shchikov,Sergio Molinari,Frédérique Motte,David John Nutter,Nicolas Peretto,Stefano Pezzuto,A. Roy,K. L. J. Rygl,Luigi Spinoglio,Glenn J. White +25 more
TL;DR: In this paper, the results from the Herschel Gould Belt survey for the B211/L1495 region in the Taurus molecular cloud were presented. And they showed that the radial density profile of B211 filament approaches a power-law behavior at large radii and exhibits a marked drop at small radii.
Journal ArticleDOI
The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types
Ilse De Looze,Diane Cormier,Vianney Lebouteiller,Suzanne C. Madden,Maarten Baes,George J. Bendo,Médéric Boquien,Alessandro Boselli,David L. Clements,Luca Cortese,Luca Cortese,Asantha Cooray,Asantha Cooray,Maud Galametz,Frédéric Galliano,Javier Graciá-Carpio,K. G. Isaak,O. Ł. Karczewski,T. J. Parkin,Eric W. Pellegrini,Aurélie Rémy-Ruyer,Luigi Spinoglio,Matthew Smith,Eckhard Sturm +23 more
TL;DR: In this paper, the authors analyzed the applicability of far-infrared fine-structure lines [Cii] 158μm, [Oi] 63μm and [Oiii] 88μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity dwarf galaxies from the Herschel Dwarf Galaxy Survey and furthermore, extended the analysis to a broad sample of galaxies of various types and metallicities in the literature.