Results 21 to 30 of about 5,114 (225)
CHEMICAL PROCESSES IN PROTOPLANETARY DISKS [PDF]
The Astrophysical Journal, 2010 24 pages, 13 figures, accepted for publication in ...
Walsh, C, Millar, TJ, Nomura, H
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Interferometry and the study of protoplanetary disks [PDF]
EPJ Web of Conferences, 2015 Interferometry offers access to scales that are unresolvable using single dish telescopes, which is especially important when investigating objects with small angular sizes, such as protoplanetary disks. This Chapter introduces the concept of interferometry, and describes the basic aspects of interferometric observations when considering long (i.e. sub-
Ilee, John David, Greaves, Jane Sophia
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Ionization and heating by X-rays and cosmic rays*
EPJ Web of Conferences, 2015 High-energy radiation from the central T Tauri and protostars plays an important role in shaping protoplanetary disks and influences their evolution. Such radiation, in particular X-rays and extreme-ultraviolet (EUV) radiation, is predominantly generated
Güdel Manuel
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The Determination of Protoplanetary Disk Masses [PDF]
, 2017 In this article we review the methods used to determine the gas and dust masses of protoplanetary disks, with an emphasis on the lesser characterized total gas mass. Our review encompasses all the indirect tracers and the methodology that is be used to isolate the hidden H2 via dust, CO, and HD emission.
Bergin, Edwin A., Williams, Jonathan P.
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Scattered Radiation of Protoplanetary Disks
Universe, 2022 Scattered radiation of circumstellar (CS) dust plays an important role in the physics of young stars. Its observational manifestations are various but more often they are connected with the appearance of intrinsic polarization in young stars and their CS
Vladimir P. Grinin +1 more
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PROTOPLANETARY DISK STRUCTURES IN OPHIUCHUS [PDF]
The Astrophysical Journal, 2009 ApJ in press: 51 pages, 13 ...
Andrews, Sean M. +4 more
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The Astrophysical Journal, 2023 We present a three-dimensional, time-dependent MHD simulation of the short-term interaction between a protoplanetary disk and the stellar corona in a T Tauri system.
Ofer Cohen +6 more
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Thermodynamics of the dead-zone inner edge in protoplanetary disks
, 2014 International audienceContext. In protoplanetary disks, the inner boundary between the turbulent and laminar regions could be a promising site for planet formation, thanks to the trapping of solids at the boundary itself or in vortices generated by the ...
Faure, Julien +5 more
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Resonant Relaxation in Protoplanetary Disks [PDF]
The Astronomical Journal, 1998 19 pages, 1 figure, LaTeX, submitted to ...
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Vortices in Protoplanetary Disks [PDF]
The Astrophysical Journal, 1999 We use a high order accuracy spectral code to carry out two-dimensional time-dependent numerical simulations of vortices in accretion disks. In particular, we examine the stability and the life time of vortices in circumstellar disks around young stellar objects. The results show that cyclonic vortices dissipate quickly, while anticyclonic vortices can
Godon, Patrick., Livio, Mario.
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