Zobrazeno 1 - 10
of 19
pro vyhledávání: '"G. S. Mathews"'
Autor:
G. S. Mathews, Karin I. Öberg, Jonathan Williams, Victoria Salinas, Michiel R. Hogerheijde, C. Qi, David J. Wilner
Publikováno v:
Astronomy & Astrophysics (0004-6361), 606, A125
Astronomy & Astrophysics (0004-6361)
Astronomy & Astrophysics, 606:A125. EDP Sciences
Astronomy & Astrophysics (0004-6361)
Astronomy & Astrophysics, 606:A125. EDP Sciences
Context. Deuterium fractionation has been used to study the thermalhistory of prestellar environments. Their formation pathways tracedifferent regions of the disk and may shed light into the physicalstructure of the disk, including locations of impor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4bbde0fbe6cbe285f255436d1b82ef73
https://doi.org/10.1051/0004-6361/201731223
https://doi.org/10.1051/0004-6361/201731223
Autor:
Markus Schmalzl, Simon Bruderer, Ewine F. van Dishoeck, Nienke van der Marel, Vincent Geers, Tim A. van Kempen, Til Birnstiel, Paola Pinilla, G. S. Mathews, Cornelis P. Dullemond, Joanna M. Brown, Gregory J. Herczeg
Publikováno v:
Proceedings of the International Astronomical Union. 8:90-93
Planet formation and clearing of protoplanetary disks is one of the long standing problems in disk evolution theory. The best test of clearing scenarios is observing systems that are most likely to be actively forming planets: the transitional disks
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d0986d285214d31548ad6cb887d766d9
https://doi.org/10.1017/s1743921313007989
https://doi.org/10.1017/s1743921313007989
Autor:
John M. Carpenter, Marco Tazzari, Juan M. Alcalá, Isa Oliveira, Giovanni P. Rosotti, E. F. van Dishoeck, Anna Miotello, Timo Prusti, A. Natta, Carlo F. Manara, G. Guidi, N. van der Marel, Megan Ansdell, Jonathan P. Williams, G. S. Mathews, Leonardo Testi
Publikováno v:
Astronomy & Astrophysics, 591, L3
NASA Astrophysics Data System
Astronomy & Astrophysics
NASA Astrophysics Data System
Astronomy & Astrophysics
A relation between the mass accretion rate onto the central young star and the mass of the surrounding protoplanetary disk has long been theoretically predicted and observationally sought. For the first time, we have accurately and homogeneously dete
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::090c696eb63d85f76200ba2e57e778de
https://doi.org/10.1051/0004-6361/201628549
https://doi.org/10.1051/0004-6361/201628549
Autor:
Yuri Aikawa, Catherine Walsh, Tilman Birnstiel, Göran Sandell, Michiel R. Hogerheijde, Gwendolyn Meeus, Attila Juhasz, Hideko Nomura, G. S. Mathews, Paola Pinilla, Daniel Harsono, Tom J. Millar, William R. F. Dent
Publikováno v:
Walsh, C, Juhasz, A, Pinilla, P, Harsono, D, S. Mathews, G, R. F. Dent, W, R. Hogerheijde, M, Birnstiel, T, Meeus, G, Nomura, H, Aikawa, Y, Millar, T J & Sandell, G 2014, ' ALMA hints at the presence of two companions in the disk around HD 100546 ', Astrophysical Journal Letters, vol. 791, L6 . https://doi.org/10.1088/2041-8205/791/1/L6
HD 100546 is a well-studied Herbig Be star-disk system that likely hosts a close-in companion with compelling observational evidence for an embedded protoplanet at 68 AU. We present ALMA observations of the HD 100546 disk which resolve the gas and du
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e60d493c6a49a67dd0fb64bf1734ba5b
Autor:
William R. F. Dent, Carlos Eiroa, David Barrado, Christophe Pinte, Gwendolyn Meeus, Jonathan Williams, S. Vicente, Inga Kamp, Jean-Charles Augereau, Pablo Riviere-Marichalar, G. S. Mathews, Gaspard Duchene, Christian D. Howard, William D. Vacca, Göran Sandell, Carol A. Grady, Francois Menard, Aki Roberge, Wing-Fai Thi, Linda Podio
Publikováno v:
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
The Astrophysical Journal, 776, 21
Astrophysical Journal, 776(1):21. IOP PUBLISHING LTD
instname
The Astrophysical Journal, 776, 21
Astrophysical Journal, 776(1):21. IOP PUBLISHING LTD
The Astrophysical Journal 776.1 (2013): 21 reproduced by permission of the AAS
The Herschel Space Observatory was used to observe ∼120 pre-main-sequence stars in Taurus as part of the GASPS Open Time Key project. Photodetector Array Camera and
The Herschel Space Observatory was used to observe ∼120 pre-main-sequence stars in Taurus as part of the GASPS Open Time Key project. Photodetector Array Camera and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b9a21598abb2e1655508e2d9e29af9c0
http://arxiv.org/abs/1308.6019
http://arxiv.org/abs/1308.6019
Autor:
Francois Menard, Kengo Tachihara, L.-Å. Nyman, P. D. Klaassen, Stuartt Corder, Leonardo Testi, Mark G. Rawlings, E. Chapillon, Satoko Takahashi, P. Cortes, N. Phillips, Eiji Akiyama, J. Rodń, T. A. van Kempen, W. R. F. Dent, Attila Juhasz, C. López, G. S. Mathews, Antonio Hales, I. de Gregorio-Monsalvo, Masao Saito, Christophe Pinte, Aya E. Higuchi
Publikováno v:
Astronomy & Astrophysics, 557, A133
Aims: The aim of this work is to study the structure of the protoplanetary disk surrounding the Herbig Ae star HD 163296. Methods: We have used high-resolution and high-sensitivity ALMA observations of the CO(3-2) emission line and the continuum at 8
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5643d6f1dd0b3bbbb9c37aec72668aac
http://arxiv.org/abs/1307.1357
http://arxiv.org/abs/1307.1357
Autor:
Ewine F. van Dishoeck, Simon Bruderer, Vincent Geers, Cornelis P. Dullemond, Til Birnstiel, Gregory J. Herczeg, Tim A. van Kempen, J. M. Brown, M. Schmalzl, Paola Pinilla, Nienke van der Marel, G. S. Mathews
The statistics of discovered exoplanets suggest that planets form efficiently. However, there are fundamental unsolved problems, such as excessive inward drift of particles in protoplanetary disks during planet formation. Recent theories invoke dust
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f747116797851044eeb3538710a9966e
http://arxiv.org/abs/1306.1768
http://arxiv.org/abs/1306.1768
Autor:
Joseph C. Mottram, Mark G. Rawlings, Daniel Harsono, E. Chapillon, G. S. Mathews, I. de Gregorio-Monsalvo, Leonardo Testi, Daniel Espada, Michiel R. Hogerheijde, P. D. Klaassen, Attila Juhasz, A. S. Hales, E. F. van Dishoeck, Satoko Takahashi
Publikováno v:
Astronomy & Astrophysics, 557, A132
The high spatial and line sensitivity of ALMA opens the possibility of resolving emission from molecules in circumstellar disks. With an understanding of physical conditions under which molecules have high abundance, they can be used as direct tracer
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::45d261226f8e11175e73f203fc9228f5
Autor:
G. S. Mathews, Pablo Riviere-Marichalar, Gwendolyn Meeus, Carlos Eiroa, Göran Sandell, Christine Chen, Aki Roberge, William R. F. Dent, François Ménard, Alexander V. Krivov, Jean-Charles Augereau, J. Donaldson
Publikováno v:
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
instname
The Astrophysical Journal 753.2 (2013): 147 reproduced by permission of the AAS
We present Herschel PACS photometry of 17 B- to M-type stars in the 30Myr old Tucana-Horologium Association. This work is part of the Herschel Open Time Key Programm
We present Herschel PACS photometry of 17 B- to M-type stars in the 30Myr old Tucana-Horologium Association. This work is part of the Herschel Open Time Key Programm
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e4cd0cb222663c09e7877bc0b637229e
https://doi.org/10.1088/0004-637x/753/2/147
https://doi.org/10.1088/0004-637x/753/2/147
Autor:
Jonathan Williams, J. Donaldson, Jean-Charles Augereau, G. S. Mathews, W. F. Thi, Gwendolyn Meeus, Francois Menard, Pablo Riviere-Marichalar, Jean-François Gonzalez, Glenn Schneider, Aki Roberge, Peter Woitke, David Barrado, Christophe Pinte, William R. F. Dent, Gaspard Duchêne, J. Lebreton, Eric Pantin, Sarah T. Maddison, Carol A. Grady, Inga Kamp
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2012, 539, pp.A17. ⟨10.1051/0004-6361/201117714⟩
Astronomy & astrophysics, 539:A17. EDP Sciences
Astronomy and Astrophysics-A&A, 2012, 539, pp.A17. ⟨10.1051/0004-6361/201117714⟩
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Astronomy and Astrophysics-A&A, EDP Sciences, 2012, 539, pp.A17. ⟨10.1051/0004-6361/201117714⟩
Astronomy & astrophysics, 539:A17. EDP Sciences
Astronomy and Astrophysics-A&A, 2012, 539, pp.A17. ⟨10.1051/0004-6361/201117714⟩
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Astronomy and Astrophysics 539 (2012): A17 reproduced with permission from Astronomy & Astrophysics
Context. HD 181327 is a young main sequence F5/F6 V star belonging to the β Pictoris moving group (age ∼ 12 Myr). It harbors an optically thin
Context. HD 181327 is a young main sequence F5/F6 V star belonging to the β Pictoris moving group (age ∼ 12 Myr). It harbors an optically thin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::743d1f328d9e485af8ce073143433a20
https://hal.archives-ouvertes.fr/hal-00686633
https://hal.archives-ouvertes.fr/hal-00686633