Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Dimitrios Stamatellos"'
Autor:
Joseph C. Mottram, Howard A. Smith, M. R. Pestalozzi, Sergio Molinari, Matthew Joseph Griffin, Jason M. Kirk, Dimitrios Stamatellos, Davide Elia, Derek Ward-Thompson, Anthony Peter Whitworth, Mark Thompson, Nicolas Peretto, Paul Martin, L. A. Wilcock, Gary A. Fuller, A. M. DiGiorgio, Eugenio Schisano, Cara Battersby
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 424:716-727
In a previous paper, we identified cores within infrared dark clouds. We regarded those without embedded sources as the least evolved and labelled them starless. Here we identify the most isolated starless cores and model them using a three-dimension
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 422:L6-L10
Autor:
Jonathan Ivor Davies, S. Linder, Anthony Peter Whitworth, Dimitrios Stamatellos, S. Roberts, Sabina Sabatini, Maarten Baes, R. Evans
Publikováno v:
New Astronomy. 10:523-533
The Monte Carlo method is a powerful tool for performing radiative equilibrium calculations, even in complex geometries. The main drawback of the standard Monte Carlo radiative equilibrium methods is that they require iteration, which makes them nume
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 424:L74-L76
We present Herschel/SPIRE observations for the 2MASS 1207334−393254 (2M1207) system. Based on radiative transfer modelling of near-infrared to submillimetre data, we estimate a disc mass of 3 ± 2 MJup and an outer disc radius of 50–100 au for th
Most stars are born in clusters and the resulting gravitational interactions between cluster members may significantly affect the evolution of circumstellar discs and therefore the formation of planets and brown dwarfs. Recent findings suggest that t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::498b0ef5194611966763c47fda7021df
http://arxiv.org/abs/1005.3017
http://arxiv.org/abs/1005.3017
Context. The fidelity of smoothed particle hydrodynamics (SPH) simulations of accretion disks depends on how artificial viscosity (AV) is formulated.\ud \ud Aims. We investigate whether standard methodology is reliable in this regard.\ud \ud Methods.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a57a91480cfd1dfdc922b1fd4a35268
https://orca.cardiff.ac.uk/id/eprint/7264/1/Controlling_artificial_viscosity_in_smoothed_particle_hydrodynamics.pdf
https://orca.cardiff.ac.uk/id/eprint/7264/1/Controlling_artificial_viscosity_in_smoothed_particle_hydrodynamics.pdf
Autor:
J. A. Rodón, K. Ganga, M. Pomarès, Friedrich Wyrowski, Mika Juvela, F. Piacentini, Melvin Hoare, William T. Reach, Stefano Pezzuto, A. Roy, Jean-Paul Baluteau, Marc-Antoine Miville-Deschenes, Russell H. Taylor, Pierre Royer, Alessio Traficante, Peter Schilke, D. Paradis, Glenn J. White, Cara Battersby, Alberto Noriega-Crespo, Harriet Parsons, M. Veneziani, Dimitrios Stamatellos, Vincent Minier, Lorenzo Piazzo, Guy S. Stringfellow, Michael G. Burton, L. K. Morgan, Frederic Schuller, F. Faustini, P. Saraceno, S. D. Lord, Jason Glenn, E. Sturm, Michael D. Smith, G. Joncas, A. M. di Giorgio, D. Polychroni, L. Montier, D. J. Marshall, N. Billot, José Cernicharo, F. Boulanger, M. T. Beltrán, Paul Martin, Matthew Joseph Griffin, B. Swinyard, Guilaine Lagache, Serena Viti, Mathieu Compiegne, Derek Ward-Thompson, P. de Bernardis, Frédérique Motte, B. Sibthorpe, Sukanya Chakrabarti, Nicolas Flagey, Christopher M. Brunt, Maggie A. Thompson, Qizhou Zhang, J.-P. Bernard, Annie Zavagno, Jean-François Robitaille, L. Spinoglio, Marc Sauvage, D. Russeil, Paolo Natoli, A. Abergel, Babar Ali, Davide Elia, D. Ikhenaode, Gary A. Fuller, C. Joblin, G. de Gasperis, Eugenio Schisano, Pedro García-Lario, Jin-Zeng Li, Isabelle Ristorcelli, Sergio Molinari, Luca Calzoletti, M. R. Pestalozzi, Nicolas Peretto, Thomas P. Robitaille, Mikako Matsuura, Riccardo Cesaroni, Rene Plume, Jan Brand, Paul F. Goldsmith, Leonardo Testi, Joseph C. Mottram, H. W. Yorke, Cristina Popescu, Martin Cohen, M. Benedettini, M. J. Barlow, Antonio Chrysostomou, Paola Caselli, Luca Olmi, Maohai Huang, Massimo Marengo, R. Paladini, Fabrizio Massi, L. A. Wilcock, Grazia Umana, Francesco Strafella, Toby J. T. Moore, Benjamin L. Schulz, R. Vavrek, T. Mueller, John Bally, J. A. D. L. Blommaert, L. D. Anderson, C. Waelkens, T. L. Lim, Richard J. Tuffs, Sean Carey, Yasuo Fukui, J. Neves, Nicola Schneider, Jason M. Kirk, Silvia Masi, Pascal André, Howard A. Smith, Luca Valenziano, Sylvain Bontemps
Publikováno v:
Scopus-Elsevier
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2010, 518, pp.L100. ⟨10.1051/0004-6361/201014659⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 518, pp.L100. ⟨10.1051/0004-6361/201014659⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2010, 518, pp.L100. ⟨10.1051/0004-6361/201014659⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 518, pp.L100. ⟨10.1051/0004-6361/201014659⟩
We present the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key-project that will map the inner Galactic Plane of the Milky Way in 5 bands. We outline our data reduction strategy and present some science high
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2cabcb6c116f3999fb26eb94f6d29b2
http://www.scopus.com/inward/record.url?eid=2-s2.0-77957835681&partnerID=MN8TOARS
http://www.scopus.com/inward/record.url?eid=2-s2.0-77957835681&partnerID=MN8TOARS