Results 21 to 30 of about 73,704 (164)

Volatiles in Protoplanetary Disks [PDF]

open access: yes, 2014
Volatiles are compounds with low sublimation temperatures, and they make up most of the condensible mass in typical planet-forming environments. They consist of relatively small, often hydrogenated, molecules based on the abundant elements carbon, nitrogen and oxygen.
Pontoppidan, K. M.   +6 more
openaire   +2 more sources

VORTEX MIGRATION IN PROTOPLANETARY DISKS [PDF]

open access: yesThe Astrophysical Journal, 2010
13 pages, 13 figures, accepted for publication in ...
Paardekooper, Sijme-Jan   +2 more
openaire   +6 more sources

The Inner Regions of Protoplanetary Disks [PDF]

open access: yesAnnual Review of Astronomy and Astrophysics, 2010
To understand how planetary systems form in the dusty disks around pre-main-sequence stars, a detailed knowledge of the structure and evolution of these disks is required. Although this is reasonably well understood for the regions of the disk beyond about 1 AU, the structure of these disks inward of 1 AU remains a puzzle. This is partly because it is
Dullemond, C. P., Monnier, J. D.
openaire   +2 more sources

Thermodynamics of the dead-zone inner edge in protoplanetary disks [PDF]

open access: yes, 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
core   +1 more source

CHEMICAL PROCESSES IN PROTOPLANETARY DISKS [PDF]

open access: yesThe Astrophysical Journal, 2010
24 pages, 13 figures, accepted for publication in ...
Walsh, C, Millar, TJ, Nomura, H
openaire   +5 more sources

Interferometry and the study of protoplanetary disks [PDF]

open access: yesEPJ 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
openaire   +4 more sources

PROTOPLANETARY DISK STRUCTURES IN OPHIUCHUS [PDF]

open access: yesThe Astrophysical Journal, 2009
ApJ in press: 51 pages, 13 ...
Andrews, Sean M.   +4 more
openaire   +2 more sources

Magnetic fields of protoplanetary disks [PDF]

open access: yes
We review the current status of studies on accretion and protoplanetary disks of young stars with large-scale magnetic fields. Observational data on magnetic fields of the disks are compiled and analysed.
Khaibrakhmanov, S. A.
core   +2 more sources

The Determination of Protoplanetary Disk Masses [PDF]

open access: yes, 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.
openaire   +2 more sources

Size-dependent charging of dust particles in protoplanetary disks

open access: yes, 2023
Context. Lightning can have a profound impact on the chemistry of planetary atmospheres. In a similar manner, as protoplanetary disks are the foundation of planet formation, the emergence of lightning in protoplanetary disks can substantially alter their
T. Balduin   +11 more
core   +1 more source

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