Zobrazeno 1 - 10
of 81
pro vyhledávání: '"L. Calzoletti"'
Autor:
Alessio Traficante, Donald F. Figer, Joachim Puls, M. M. Rubio-Díez, Jon O. Sundqvist, L. Calzoletti, Francisco Najarro
We probe the radial clumping stratification of OB stars in the intermediate and outer wind regions (r>~2 R*) to derive upper limits for mass-loss rates, and compare to current mass-loss implementation. Together with archival multi-wavelength data, ou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::46e0e0f022246c1a0a775bd86fa5e102
http://arxiv.org/abs/2108.11734
http://arxiv.org/abs/2108.11734
Akademický článek
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Autor:
A. Traficante, L. Calzoletti, M. Veneziani, B. Ali, G. de Gasperis, A. M. Di Giorgio, F. Faustini, D. Ikhenaode, S. Molinari, P. Natoli, M. Pestalozzi, S. Pezzuto, F. Piacentini, L. Piazzo, G. Polenta, E. Schisano
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 416:2932-2943
We present the data reduction pipeline for the Hi-GAL survey. Hi-GAL is a key project of the Herschel satellite which is mapping the inner part of the Galactic plane (|l
Autor:
L. K. Lundin, Per Bjerkeli, Mario Tafalla, S. Antoniucci, E. F. van Dishoeck, A. Lorenzani, Brunella Nisini, Teresa Giannini, G. Santangelo, S. Cabrit, L. Calzoletti, René Liseau, C. Codella, David A. Neufeld
Publikováno v:
Astronomy & Astrophysics, 569, L8
Context: Herschel observations suggest that the H$_2$O distribution in outflows from low-mass stars resembles the H$_2$ emission. It is still unclear which of the different excitation components that characterise the mid- and near-IR H$_2$ distributi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::374af8beebf18ea3e62342fa2ac15185
https://doi.org/10.1051/0004-6361/201424748
https://doi.org/10.1051/0004-6361/201424748
Autor:
Alessio Traficante, Jason M. Kirk, F. Faustini, P. Martin, J. A. Rodón, L. A. Montier, Frédérique Motte, R. Plume, Derek Ward-Thompson, C. Lenfestey, Maria T. Beltrán, L. Calzoletti, Sergio Molinari, Nicolas Peretto, Howard A. Smith, J.-P. Bernard, Gary A. Fuller, L. D. Anderson, Cara Battersby, M. Veneziani, I. Ristorcelli, A. M. DiGiorgio, John Bally, D. J. Marshall, L. A. Wilcock
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 518, ⟨10.1051/0004-6361/201014652⟩
Scopus-Elsevier
Astronomy and Astrophysics-A&A, 2010, 518, ⟨10.1051/0004-6361/201014652⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 518, ⟨10.1051/0004-6361/201014652⟩
Scopus-Elsevier
Astronomy and Astrophysics-A&A, 2010, 518, ⟨10.1051/0004-6361/201014652⟩
Infrared dark clouds (IRDCs) are cold and dense reservoirs of gas potentially available to form stars. Many of these clouds are likely to be pristine structures representing the initial conditions for star formation. The study presented here aims to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20a90762fcd441f8a17ad40bd8399a5f
Autor:
Yancy L. Shirley, Cara Battersby, M. Veneziani, Sergio Molinari, Frédérique Motte, Annie Zavagno, Alessio Traficante, Peter Schilke, Wayne Schlingman, A. M. DiGiorgio, Adam Ginsburg, J. A. Rodón, Q. Nguyen-Luong, Jin-Zeng Li, John Bally, Leonardo Testi, M. R. Pestalozzi, R. Plume, F. Faustini, Guy S. Stringfellow, N. Schneider-Bontemps, L. D. Anderson, L. Calzoletti
Publikováno v:
aap
aap, 2010, 518, pp.L90. ⟨10.1051/0004-6361/201014596⟩
Scopus-Elsevier
aap, 2010, 518, pp.L90. ⟨10.1051/0004-6361/201014596⟩
Scopus-Elsevier
Aims: To explore the infrared and radio properties of one of the closest Galactic starburst regions. Methods: Images obtained with the Herschel Space Observatory at wavelengths of 70, 160, 250, 350, and 500 microns using the PACS and SPIRE arrays are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0a292fa2d9c134ab5f85d66d1135de96
https://hal.science/hal-03562114
https://hal.science/hal-03562114
Autor:
Brunella Nisini, Teresa Giannini, J. Eislöffel, Dirk Froebrich, A. Caratti o Garatti, L. Calzoletti
We present a multi-epoch (20 years baseline) kinematical investigation of HH52, 53, and 54 at optical and near-IR wavelengths, along with medium and high- resolution spectroscopic analyses, probing the kinematical and physical time variability condit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78f37690ac319dfabb5a29632526761b
Autor:
Michael D. Smith, L. Calzoletti, C. J. Davis, Jochen Eisloeffel, Brunella Nisini, Teresa Giannini
We aim to characterise the morphology and the physical parameters governing the shock physics of the Herbig-Haro object HH99B. We have obtained SINFONI-SPIFFI IFU spectroscopy between 1.10 and 2.45 um detecting more than 170 emission lines, Most of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b3f06b1181453f4a8557afb9f3450eb2
Akademický článek
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Akademický článek
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