Results 31 to 40 of about 36,511 (156)
First evidence for dusty disks around Herbig Be stars
, 2003 We have carried out a high-sensitivity search for circumstellar disks around
Herbig Be stars in the continuum at 1.4mm and 2.7mm using the IRAM
interferometer at the Plateau de Bure (PdBI) .A. Fuente, A. Natta, A. Rodrguez-Franco, Curiel S., Fuente A., Girart J. M., L. Testi, Leinert C., R. Bachiller, R. Neri, The P. S. +10 morecore +1 more sourceMeasuring the mass accretion rates of Herbig Ae/Be stars with X-shooter [PDF]
, 2012 We present the results of our observations of eight magnetic Herbig Ae/Be
stars obtained with the X-shooter spectrograph mounted on UT2 at the VLT.Ardila, Bibo, Bohm, Calvet, Calvet, Catala, Coulson, D'Alessio, D'Alessio, Dahm, Donehew, Fang, Finkenzeller, Garcia, Garcia Lopez, Gatti, Grady, Grady, Grady, Grinin, Gullbring, Henning, Herbig, Herczeg, Hillenbrand, Hubrig, Hubrig, Hubrig, Hubrig, Mendigutia, Mendigutia, Mohanty, Montesinos, Mottram, Muzerolle, Muzerolle, Müller, Natta, Natta, Nguyen, Oudmaijer, Palla, Pogodin, Pogodin, Rigliaco, Tout, Tout, Wade, White +48 morecore +2 more sourcesThe First Detailed Look at a Brown Dwarf Disk
, 2003 The combination of mid-infrared and recent submm/mm measurements allows us to
set up the first comprehensive spectral energy distribution (SED) of the
circumstellar material around a young Brown Dwarf.C. P. Dullemond, Comeron F., D. Apai, I. Pascucci, Itoh Y., Manske V., Persi P., Th. Henning +7 morecore +1 more sourceThe origin of hydrogen line emission for five Herbig Ae/Be stars
spatially resolved by VLTI/AMBER spectro-interferometry [PDF]
, 2008 To trace the accretion and outflow processes around YSOs, diagnostic spectral
lines such as the BrG 2.166 micron line are widely used, although due to a lack
of spatial resolution, the origin of the line emission is still unclear.A. Isella, A. Meilland, A. Natta, Acke, Acke, Antoniucci, Bacciotti, Benedettini, Blandford, Blondel, Borges Fernandes, Brittain, Böhm, Cabrit, Calvet, Catala, Catala, Cidale, Coffey, Corcoran, D. Schertl, de Winter, Donati, Drew, Dullemond, E. Tatulli, Eisner, Eisner, Evans, F. Malbet, Ferreira, Ferreira, Finkenzeller, Finkenzeller, G. Weigelt, Garcia Lopez, Grady, Grady, Grady, Habart, Hartigan, Henning, Higdon, Hutsemekers, Isella, Isella, J.-P. Berger, K.-H. Hofmann, Kraus, L. Testi, Leinert, M. Benisty, M. Smith, Malbet, Malfait, Mannings, Mathis, Mestel, Millan-Gabet, Monnier, Monnier, Monnier, Muzerolle, Muzerolle, Muzerolle, Muzerolle, N. Nardetto, Natta, Natta, Nisini, O. Chesneau, Oudmaijer, P. Stee, Petrov, Pogodin, Pudritz, Richichi, S. Kraus, Shu, Sim, Sorelli, Stee, Strafella, T. Preibisch, Tannirkulam, Tatulli, Tatulli, Testi, van Boekel, van den Ancker, van den Ancker, van den Bergh, Vinkovic, Walker, Wang, Wassell, Weigelt +96 morecore +6 more sourcesSurvival of the mm-cm size grain population observed in protoplanetary
disks
, 2007 Millimeter interferometry provides evidence for the presence of mm to cm size
"pebbles" in the outer parts of disks around pre-main-sequence stars. The
observations suggest that large grains are produced relatively early in disk
evolution (< 1 Myr) and ...A. Johansen, A. Natta, Acke, Alexander, Alexander, Balbus, Balbus, Barge, Beckwith, Blum, Brandenburg, C. P. Dullemond, Cuzzi, Dubrulle, Dullemond, Dullemond, F. Brauer, Fromang, Garaud, Goldreich, Gómez, H. Klahr, Haghighipour, Hartmann, Johansen, Johansen, Johansen, Kempf, Kitamura, Klahr, Klahr, Klahr, Meeus, Nakagawa, Natta, Ormel, Rice, Rodmann, Schräpler, Sekiya, Shakura, Suttner, Takeuchi, Takeuchi, Testi, Th. Henning, Völk, Weidenschilling, Weidenschilling, Weidenschilling, Weidenschilling, Weidenschilling, Wilner, Wolf, Youdin, Youdin, Youdin +56 morecore +1 more sourceMarie-Christine Natta, Baudelaire [PDF]
Studi Francesi, 2018 Il nome di Baudelaire e talmente noto e carico di rapporti e suggestioni, specialmente nel contesto della cosiddetta “modernita”, che costituisce una sicura attrazione per un ampio pubblico. Avvalendosi della sua competenza in tema di dandysme (si ricordi almeno il libro La Grandeur sans convictions.openaire +2 more sourcesThe dusty disk around VV Ser
, 2008 We have carried out observations at millimeter and centimeter wavelengths
towards VV Ser using the Plateau de Bure Interferometer and the Very Large
Array. This allows us to compute the SED from near infrared to centimeter
wavelengths.A. Fuente, Chavarria K., C., L. Testi, Leinert C., P. Planesas, R. Bachiller, R. Neri, Straizys V., T. Alonso‐Albi +8 morecore +1 more sourceEffects of scattering and dust grain size on the temperature structure
of protoplanetary discs: A three-layer approach
, 2008 The temperature in the optically thick interior of protoplanetary discs is
essential for the interpretation of millimeter observations of the discs, for
the vertical structure of the discs, for models of the disc evolution and the
planet formation, and ...Akinori Oka, Akio K. Inoue, Calvet, Chiang, Chiang, D'Alessio, Draine, Draine, Dullemond, Dullemond, Dullemond, Dullemond, Dullemond, Garaud, Miyake, Ng, Nomura, Olson, Pascucci, Rafikov, Rybicki, Sano, Sasselov, Steinacker, Taishi Nakamoto +24 morecore +1 more sourcePOISSON project - I - Emission lines as accretion tracers in young
stellar objects: results from observations of Chamaeleon I and II sources
, 2011 We present the results of the analysis of LR optical-NIR spectra (0.6-2.4 um)
of a sample 47 YSOs in the ChaI and II star-forming clouds. These data are part
of the POISSON project (Protostellar Optical-Infrared Spectral Survey on NTT).Antoniucci, S., Bacciotti, F., Cabrit, S., Dougados, C., Eisloeffel, J., Garatti, A. Caratti o, Giannini, T., Lopez, R. Garcia, Lorenzetti, D., Nisini, B., Ray, T. +10 morecore +3 more sourcesOn the properties of discs around accreting brown dwarfs
, 2010 We present a grid of models of accreting brown dwarf systems with
circumstellar discs. The calculations involve a self-consistent solution of
both vertical hydrostatic and radiative equilibrium along with a sophisticated
treatment of dust sublimation. We Allen, Allers, Anders, Asplund, Barrado y Navascués, Bertout, Bessell, Bessell, Bessell, Bessell, Bouvier, Bouvier, Bouy, Bryden, Camenzind, Carpenter, Chabrier, Clarke, Cohen, Cohen, Currie, Dahm, Dullemond, Elias, Ercolano, Fukugita, Gatti, Griffin, Griffin, Gullbring, Gutermuth, Haisch, Harries, Harries, Hartmann, Hawarden, Herbst, Herczeg, Holland, Isella, Jayawardhana, Joergens, Johnson, Kama, Kennedy, Kenyon, Koenigl, Kurosawa, Kurosawa, Lada, Lada, Leggett, Lucy, Luhman, Luhman, Luhman, Martín, Mayne, Mayne, Meyer, Mohanty, Mohanty, Monin, Morrow, Muzerolle, Muzerolle, Najita, Nathan J. Mayne, Natta, Natta, Natta, Neugebauer, Noels, Pascucci, Pinte, Poglitsch, Pollack, Rice, Robitaille, Scholz, Scholz, Shakura, Shu, Siess, Siess, Simons, Skrutskie, Stephens, Tannirkulam, Tim J. Harries, Tokunaga, Tout, Walker, White, Wood, Zapatero Osorio +95 morecore +1 more source
