Zobrazeno 1 - 6
of 6
pro vyhledávání: '"L. A. Wilcock"'
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
Autor:
Dimitris Stamatellos, A. M. DiGiorgio, Jason M. Kirk, Gary A. Fuller, Derek Ward-Thompson, Rene Plume, Eugenio Schisano, Joseph C. Mottram, Howard A. Smith, Matthew Joseph Griffin, Davide Elia, M. R. Pestalozzi, Sergio Molinari, Pierrick Martin, Maggie A. Thompson, L. A. Wilcock, A. P. Whitworth, Nicolas Peretto
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 422:1071-1082
We have used data taken as part of the Herschel infrared Galactic Plane survey (Hi-GAL) to study 3171 infrared-dark cloud (IRDC) candidates that were identified in the mid-infrared (8 {\mu}m) by Spitzer (we refer to these as 'Spitzer-dark' regions).
Autor:
Jason M. Kirk, Sergio Molinari, Derek Ward-Thompson, Dimitris Stamatellos, Anthony Peter Whitworth, B. Sibthorpe, Matthew Joseph Griffin, L. A. Wilcock
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 409:12-21
We demonstrate the use of the 3D Monte Carlo radiative transfer code PHAETHON to model infrared-dark clouds (IRDCs) that are externally illuminated by the interstellar radiation field (ISRF). These clouds are believed to be the earliest observed phas
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:
Dimitris Stamatellos, Gary A. Fuller, Joseph C. Mottram, Rene Plume, Paul Martin, L. A. Wilcock, Matthew Joseph Griffin, Derek Ward-Thompson, Sergio Molinari, Christopher M. Brunt, Mark Thompson, Cara Battersby, Jason M. Kirk, Anthony Peter Whitworth, Howard A. Smith, Nicolas Peretto
Publikováno v:
Astronomy & Astrophysics. 526:A159
The densest infrared dark clouds (IRDCs) may represent the earliest observable stage of high-mass star formation. These clouds are very cold, hence they emit mainly at far-infrared and sub-mm wavelengths. For the first time, Herschel has provided mul
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