Zobrazeno 1 - 10
of 52
pro vyhledávání: '"Tilling, I."'
Autor:
Dent, W. R. F., Thi, W. F., Kamp, I., Williams, J. P., Menard, F., Andrews, S., Ardila, D., Aresu, G., Augereau, J-C., Navascues, D. Barrado y, Brittain, S., Carmona, A., Ciardi, D., Danchi, W., Donaldson, J., Duchene, G., Eiroa, C., Fedele, D., Grady, C., de Gregorio-Molsalvo, I., Howard, C., Huelamo, N., Krivov, A., Lebreton, J., Liseau, R., Martin-Zaidi, C., Mathews, G., Meeus, G., Mendigutia, I., Montesinos, B., Morales-Calderon, M., Mora, A., Nomura, H., Pantin, E., Pascucci, I., Phillips, N., Pinte, C., Podio, L., Ramsay, S. K., Riaz, B., Riviere-Marichalar, P., Roberge, A., Sandell, G., Solano, E., Tilling, I., Torrelles, J. M., Vandenbusche, B., Vicente, S., White, G. J., Woitke, P.
GASPS is a far-infrared line and continuum survey of protoplanetary and young debris disks using PACS on the Herschel Space Observatory. The survey includes [OI] at 63 microns, as well as 70, 100 and 160um continuum, with the brightest objects also s
Externí odkaz:
http://arxiv.org/abs/1306.0275
Autor:
Tilling, I., Woitke, P., Meeus, G., Mora, A., Montesinos, B., Riviere-Marichalar, P., Eiroa, C., Thi, W. -F., Isella, A., Roberge, A., Martin-Zaidi, C., Kamp, I., Pinte, C., Sandell, G., Vacca, W. D., Ménard, F., Mendigutía, I., Duchêne, G., Dent, W. R. F., Aresu, G., Meijerink, R., Spaans, M.
We present detailed model fits to observations of the disc around the Herbig Ae star HD 163296. This well-studied object has an age of ~ 4 Myr, with evidence of a circumstellar disc extending out to ~ 540AU. We use the radiation thermo-chemical disc
Externí odkaz:
http://arxiv.org/abs/1111.2549
Autor:
Kamp, I., Woitke, P., Pinte, C., Tilling, I., Thi, W. -F., Menard, F., Duchene, G., Augereau, J. -C.
Aims. We want to understand the chemistry and physics of disks on the basis of a large unbiased and statistically relevant grid of disk models. One of the main goals is to explore the diagnostic power of various gas emission lines and line ratios for
Externí odkaz:
http://arxiv.org/abs/1103.5763
Autor:
Mathews, G. S., Dent, W. R. F., Williams, J. P., Howard, C. D., Meeus, G., Riaz, B., Roberge, A., Sandell, G., Vandenbussche, B., Duchêne, G., Kamp, I., Ménard, F., Montesinos, B., Pinte, C., Thi, W. F., Woitke, P., Alacid, J. M., Andrews, S. M., Ardila, D. R., Aresu, G., Augereau, J. C., Barrado, D., Brittain, S., Ciardi, D. R., Danchi, W., Eiroa, C., Fedele, D., Grady, C. A., de Gregorio-Monsalvo, I., Heras, A., Huelamo, N., Krivov, A., Lebreton, J., Liseau, R., Martin-Zaidi, C., Mendigutía, I., Mora, A., Morales-Calderon, M., Nomura, H., Pantin, E., Pascucci, I., Phillips, N., Podio, L., Poelman, D. R., Ramsay, S., Rice, K., Riviere-Marichalar, P., Solano, E., Tilling, I., Walker, H., White, G. J., Wright, G., Collaboration, the GASPS
Context - Circumstellar discs are ubiquitous around young stars, but rapidly dissipate their gas and dust on timescales of a few Myr. The Herschel space observatory allows for the study of the warm disc atmosphere, using far-infrared spectroscopy to
Externí odkaz:
http://arxiv.org/abs/1005.3864
Autor:
Pinte, C., Woitke, P., Menard, F., Duchene, G., Kamp, I., Meeus, G., Mathews, G. S., Howard, C. D., Grady, C. A., Thi, W. -F., Tilling, I., Augereau, J. -C., Dent, W. R. F., Alacid, J. M., Andrews, S., Ardila, D. R., Aresu, G., Barrado, D., Brittain, S., Ciardi, D. R., Danchi, W., Eiroa, C., Fedele, D., de Gregorio-Monsalvo, I., Heras, A., Huelamo, N., Krivov, A., Lebreton, J., Liseau, R., Martin-Zaidi, C., Mendigutia, I., Montesinos, B., Mora, A., Morales-Calderon, M., Nomura, H., Pantin, E., Pascucci, I., Phillips, N., Podio, L., Poelman, D. R., Ramsay, S., Riaz, B., Rice, K., Riviere-Marichalar, P., Roberge, A., Sandell, G., Solano, E., Vandenbussche, B., Walker, H., Williams, J. P., White, G. J., Wright, G.
The Herschel GASPS Key Program is a survey of the gas phase of protoplanetary discs, targeting 240 objects which cover a large range of ages, spectral types, and disc properties. To interpret this large quantity of data and initiate self-consistent a
Externí odkaz:
http://arxiv.org/abs/1005.3826
Autor:
Thi, W. F., Mathews, G., Ménard, F., Woitke, P., Meeus, G., Riviere-Marichalar, P., Pinte, C., Howard, C. D., Roberge, A., Sandell, G., Pascucci, I., Riaz, B., Grady, C. A., Dent, W. R. F., Kamp, I., Duchêne, G., Augereau, J. C., Pantin, E., Vandenbussche, B., Tilling, I., Williams, J. P., Eiroa, C., Barrado, D., Alacid, J. M., Andrews, S., Ardila, D. R., Aresu, G., Brittain, S., Ciardi, D. R., Danchi, W., Fedele, D., de Gregorio-Monsalvo, I., Heras, A., Huelamo, N., Krivov, A., Lebreton, J., Liseau, R., Martin-Zaidi, C., Mendigutía, I., Montesinos, B., Mora, A., Morales-Calderon, M., Nomura, H., Phillips, N., Podio, L., Poelman, D. R., Ramsay, S., Rice, K., Solano, E., Walker, H., White, G. J., Wright, G.
Planets are formed in disks around young stars. With an age of ~10 Myr, TW Hya is one of the nearest T Tauri stars that is still surrounded by a relatively massive disk. In addition a large number of molecules has been found in the TW Hya disk, makin
Externí odkaz:
http://arxiv.org/abs/1005.3830
Autor:
Meeus, G., Pinte, C., Woitke, P., Montesinos, B., Mendigutía, I., Riviere-Marichalar, P., Eiroa, C., Mathews, G. S., Vandenbussche, B., Howard, C. D., Roberge, A., Sandell, G., Duchêne, G., Ménard, F., Grady, C. A., Dent, W. R. F., Kamp, I., Augereau, J. C., Thi, W. F., Tilling, I., Alacid, J. M., Andrews, S., Ardila, D. R., Aresu, G., Barrado, D., Brittain, S., Ciardi, D. R., Danchi, W., Fedele, D., de Gregorio-Monsalvo, I., Heras, A., Huelamo, N., Krivov, A., Lebreton, J., Liseau, R., Martin-Zaidi, C., Mora, A., Morales-Calderon, M., Nomura, H., Pantin, E., Pascucci, I., Phillips, N., Podio, L., Poelman, D. R., Ramsay, S., Riaz, B., Rice, K., Solano, E., Walker, H., White, G. J., Williams, J. P., Wright, G., Collaboration, the GASPS
In an effort to simultaneously study the gas and dust components of the disc surrounding the young Herbig Ae star HD 169142, we present far-IR observations obtained with the PACS instrument onboard the Herschel Space Observatory. This work is part of
Externí odkaz:
http://arxiv.org/abs/1005.3828
Methods. We use the recently developed disk code ProDiMo to calculate the physico-chemical structure of protoplanetary disks and apply the Monte-Carlo line radiative transfer code RATRAN to predict observable line profiles and fluxes. We consider a s
Externí odkaz:
http://arxiv.org/abs/0911.1949
We investigate the evolution of accretion luminosity $L_{\rm acc}$ and stellar luminosity ${L_\ast}$ in pre-mainsequence stars. We make the assumption that when the star appears as a Class II object, the major phase of accretion is long past, and the
Externí odkaz:
http://arxiv.org/abs/0801.2100
Autor:
Dent, W. R. F., Thi, W. F., Kamp, I., Williams, J. P., Menard, F., Andrews, S., Ardila, D., Aresu, G., Augereau, J. -C., Barrado y Navascues, D., Brittain, S., Carmona, A., Ciardi, D., Danchi, W., Donaldson, J., Duchene, G., Eiroa, C., Fedele, D., Grady, C., de Gregorio-Molsalvo, I., Howard, C., Huelamo, N., Krivov, A., Lebreton, J., Liseau, R., Martin-Zaidi, C., Mathews, G., Meeus, G., Mendigutia, I., Montesinos, B., Morales-Calderon, M., Mora, A., Nomura, H., Pantin, E., Pascucci, I., Phillips, N., Pinte, C., Podio, L., Ramsay, S. K., Riaz, B., Riviere-Marichalar, P., Roberge, A., Sandell, G., Solano, E., Tilling, I., Torrelles, J. M., Vandenbusche, B., Vicente, S., White, G. J., Woitke, P.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 125(927), 477-505
We describe a large-scale far-infrared line and continuum survey of protoplanetary disk through to young debris disk systems carried out using the ACS instrument on the Herschel Space Observatory. This Open Time Key program, known as GASPS (Gas Surve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::98b93911118f06933ed517215be33eec
https://research.rug.nl/en/publications/3178bde8-56f5-4913-a5f6-0a44e8950863
https://research.rug.nl/en/publications/3178bde8-56f5-4913-a5f6-0a44e8950863