Zobrazeno 1 - 10
of 1 059
pro vyhledávání: '"PILBRATT, G. L."'
Autor:
Elia, D., Merello, M., Molinari, S., Schisano, E., Zavagno, A., Russeil, D., Mège, P., Martin, P. G., Olmi, L., Pestalozzi, M., Plume, R., Ragan, S. E., Benedettini, M., Eden, D. J., Moore, T. J. T., Noriega-Crespo, A., Paladini, R., Palmeirim, P., Pezzuto, S., Pilbratt, G. L., Rygl, K. L. J., Schilke, P., Strafella, F., Tan, J. C., Traficante, A., Baldeschi, A., Bally, J., di Giorgio, A. M., Fiorellino, E., Liu, S. J., Piazzo, L., Polychroni, D.
We present the $360^\circ$ catalogue of physical properties of Hi-GAL compact sources, detected between 70 and 500 $\mu$m. This release not only completes the analogous catalogue previously produced by the Hi-GAL collaboration for $-71^\circ \lesssim
Externí odkaz:
http://arxiv.org/abs/2104.04807
Autor:
Elia, D., Molinari, S., Schisano, E., Pestalozzi, M., Pezzuto, S., Merello, M., Noriega-Crespo, A., Moore, T. J. T., Russeil, D., Mottram, J. C., Paladini, R., Strafella, F., Benedettini, M., Bernard, J. P., Di Giorgio, A., Eden, D. J., Fukui, Y., Plume, R., Bally, J., Martin, P. G., Ragan, S. E., Jaffa, S. E., Motte, F., Olmi, L., Schneider, N., Testi, L., Wyrowski, F., Zavagno, A., Calzoletti, L., Faustini, F., Natoli, P., Palmerim, P., Piacentini, F., Piazzo, L., Pilbratt, G. L., Polychroni, D., Baldeschi, A., Beltrán, M. T., Billot, N., Cambrésy, L., Cesaroni, R., García-Lario, P., Hoare, M. G., Huang, M., Joncas, G., Liu, S. J., Maiolo, B. M. T., Marsh, K. A., Maruccia, Y., Mège, P., Peretto, N., Rygl, K. L. J., Schilke, P., Thompson, M. A., Traficante, A., Umana, G., Veneziani, M., Ward-Thompson, D., Whitworth, A. P., Arab, H., Bandieramonte, M., Becciani, U., Brescia, M., Buemi, C., Bufano, F., Butora, R., Cavuoti, S., Costa, A., Fiorellino, E., Hajnal, A., Hayakawa, T., Kacsuk, P., Leto, P., Causi, G. Li, Marchili, N., Martinavarro-Armengol, S., Mercurio, A., Molinaro, M., Riccio, G., Sano, H., Sciacca, E., Tachihara, K., Torii, K., Trigilio, C., Vitello, F., Yamamoto, H.
Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 $\mu$m. We present a band-merged catalogue of spatially matched sources and their properties derived from fits to the sp
Externí odkaz:
http://arxiv.org/abs/1706.01046
Autor:
Rigopoulou, D., Helmich, F., Hunt, L., Goicoechea, J., Hartogh, P., Fedele, D., Matsuura, M., Spinoglio, L., Elbaz, D., Griffin, M., Pilbratt, G. L., Chapillon, E.
The European Far-Infrared (FIR) Space Roadmap focuses on fundamental, yet still unresolved, astrophysical questions that can only be answered through a far-infrared space mission and gives an overview of the technology required to answer them. The do
Externí odkaz:
http://arxiv.org/abs/1701.00366
Autor:
Montesinos, B., Eiroa, C., Krivov, A. V., Marshall, J. P., Pilbratt, G. L., Liseau, R., Mora, A., Maldonado, J., Wolf, S., Ertel, S., Bayo, A., Augereau, J. -C., Heras, A. M., Fridlund, M., Danchi, W. C., Solano, E., Kirchschlager, F., del Burgo, C., Montes, D.
Publikováno v:
A&A 593, A51 (2016)
Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems. Their solar system's counterparts are the asteroid and Edgeworth-Kuiper belts. The aim of this paper is to provide robust numbers
Externí odkaz:
http://arxiv.org/abs/1605.05837
Autor:
Brandeker, A., Cataldi, G., Olofsson, G., Vandenbussche, B., Acke, B., Barlow, M. J., Blommaert, J. A. D. L., Cohen, M., Dent, W. R. F., Dominik, C., Di Francesco, J., Fridlund, M., Gear, W. K., Glauser, A. M., Greaves, J. S., Harvey, P. M., Heras, A. M., Hogerheijde, M. R., Holland, W. S., Huygen, R., Ivison, R. J., Leeks, S. J., Lim, T. L., Liseau, R., Matthews, B. C., Pantin, E., Pilbratt, G. L., Royer, P., Sibthorpe, B., Waelkens, C., Walker, H. J.
Publikováno v:
A&A 591, A27 (2016)
The young star beta Pictoris is well known for its dusty debris disk, produced through the grinding down by collisions of planetesimals, kilometre-sized bodies in orbit around the star. In addition to dust, small amounts of gas are also known to orbi
Externí odkaz:
http://arxiv.org/abs/1604.07418
Autor:
Molinari, S., Schisano, E., Elia, D., Pestalozzi, M., Traficante, A., Pezzuto, S., Swinyard, B. M., Noriega-Crespo, A., Bally, J., Moore, T. J. T., Plume, R., Zavagno, A., di Giorgio, A. M., Liu, S. J., Pilbratt, G. L., Mottram, J. C., Russeil, D., Piazzo, L., Veneziani, M., Benedettini, M., Calzoletti, L., Faustini, F., Natoli, P., Piacentini, F., Merello, M., Palmese, A., Del Grande, R., Polychroni, D., Rygl, K. L. J., Polenta, G., Barlow, M. J., Bernard, J. -P., Martin, P. G., Testi, L., Ali, B., Andrè, P., Beltrán, M. T., Billot, N., Brunt, C., Carey, S., Cesaroni, R., Compiègne, M., Eden, D., Fukui, Y., Garcia-Lario, P., Hoare, M. G., Huang, M., Joncas, G., Lim, T. L., Lord, S. D., Martinavarro-Armengol, S., Motte, F., Paladini, R., Paradis, D., Peretto, N., Robitaille, T., Schilke, P., Schneider, N., Schulz, B., Sibthorpe, B., Strafella, F., Thompson, M. A., Umana, G., Ward-Thompson, D., Wyrowski, F.
(Abridged) We present the first public release of high-quality data products (DR1) from Hi-GAL, the {\em Herschel} infrared Galactic Plane Survey. Hi-GAL is the keystone of a suite of continuum Galactic Plane surveys from the near-IR to the radio, an
Externí odkaz:
http://arxiv.org/abs/1604.05911
Publikováno v:
A&A 578, A23 (2015)
New data from the Herschel Space Observatory are broadening our understanding of the physics and evolution of the outer regions of protoplanetary disks in star forming regions. In particular they prove to be useful to identify transitional disk candi
Externí odkaz:
http://arxiv.org/abs/1501.05204
Autor:
de Oliveira, C. Alves, Schneider, N., Merín, B., Prusti, T., Ribas, Á., Cox, N. L. J., Vavrek, R., Könyves, V., Arzoumanian, D., Puga, E., Pilbratt, G. L., Kóspál, Á., André, Ph., Didelon, P., Men'shchikov, A., Royer, R., Waelkens, C., Bontemps, S., Winston, E., Spezzi, L.
Publikováno v:
A&A 568, A98 (2014)
The Chamaeleon molecular cloud complex is one of the nearest star-forming sites encompassing three molecular clouds with a different star-formation history, from quiescent (Cha III) to actively forming stars (Cha II), and reaching the end of star-for
Externí odkaz:
http://arxiv.org/abs/1404.6526
Autor:
Marshall, J. P., Moro-Martín, A., Eiroa, C., Kennedy, G., Mora, A., Sibthorpe, B., Lestrade, J. -F., Maldonado, J., Sanz-Forcada, J., Wyatt, M. C., Matthews, B., Horner, J., Montesinos, B., Bryden, G., del Burgo, C., Greaves, J. S., Ivison, R. J., Meeus, G., Olofsson, G., Pilbratt, G. L., White, G. J.
The $\textit{Herschel}$ DEBRIS, DUNES and GT programmes observed 37 exoplanet host stars within 25 pc at 70, 100 and 160 $\mu$m with the sensitivity to detect far-infrared excess emission at flux density levels only an order of magnitude greater than
Externí odkaz:
http://arxiv.org/abs/1403.6186
Autor:
Wiegert, J., Liseau, R., Thébault, P., Olofsson, G., Mora, A., Bryden, G., Marshall, J. P., Eiroa, C., Montesinos, B., Ardila, D., Augereau, J. C., Aran, A. Bayo, Danchi, W. C., del Burgo, C., Ertel, S., Fridlund, M. C. W., Hajigholi, M., Krivov, A. V., Pilbratt, G. L., Roberge, A., White, G. J., Wolf, S.
[Abridged] Debris discs around main-sequence stars indicate the presence of larger rocky bodies. The components of the nearby binary aCentauri have higher than solar metallicities, which is thought to promote giant planet formation. We aim to determi
Externí odkaz:
http://arxiv.org/abs/1401.6896