Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Ayano Komaki"'
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 2, p 81 (2024)
We perform radiation hydrodynamics simulations to study the structure and evolution of a photoevaporating protoplanetary disk. Ultraviolet and X-ray radiation from the host star heats the disk surface, where H _2 pumping also operates efficiently. We
Externí odkaz:
https://doaj.org/article/ff756137336d4863bf121a265bcb313d
Publikováno v:
Proceedings of the International Astronomical Union. 16:294-299
Photoelectric effect of dust grains by UV radiation is an important process for disk heating, but as a disk evolves, the amount of dust grains decreases. Photoeaporation is a disk dispersal process, which is caused by high-energy radiation. We perfor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2eb2289a4eb9dd127e8b44b2e6d7a9ba
https://doi.org/10.1017/s1743921322001296
https://doi.org/10.1017/s1743921322001296
Unbiased understanding of molecular distributions in a disk/envelope system of a low-mass protostellar source is crucial for investigating physical and chemical evolution processes. We have observed 23 molecular lines toward the Class 0 protostellar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::80341cb5fd85a7a66c0e3c7fffd98064
http://arxiv.org/abs/2110.00150
http://arxiv.org/abs/2110.00150
Publikováno v:
The Astrophysical Journal. 910:51
Recent multi-wavelength observations suggest that inner parts of protoplanetary disks (PPDs) have shorter lifetimes for heavier host stars. Since PPDs around high-mass stars are irradiated by strong ultra-violet radiation, photoevaporation may provid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1c65cf4dad6f98d5296b1bb2cb0e45e2
https://doi.org/10.3847/1538-4357/abe2af
https://doi.org/10.3847/1538-4357/abe2af
Publikováno v:
Astrophysical Journal; 3/10/2024, Vol. 963 Issue 2, p1-9, 9p
Publikováno v:
Astrophysical Journal; 3/20/2021, Vol. 910 Issue 1, p1-11, 11p