Self-scattering on large, porous grains in protoplanetary disks with dust settling

被引：0
|
作者：
Brunngräber, R. [1 ]
Wolf, S. [1 ]
机构：
[1] Institut für Theoretische Physik und Astrophysik, Christian-Albrechts-Universität zu Kiel, Leibnizstr. 15, Kiel,24118, Germany
来源：
Astronomy and Astrophysics | 2021年 / 648卷
关键词：
Millimeter waves - Monte Carlo methods - Porosity - Grain size and shape - Dust - Optical properties - Radiative transfer;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
引用
收藏
相关论文
共 50 条
  • [31] Evolution of porous dust grains in protoplanetary discs - I. Growing grains
    Garcia, Anthony J. L.
    Gonzalez, Jean-Francois
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 493 (02) : 1788 - 1800
  • [32] Co-evolution of dust grains and protoplanetary disks. II. Structure and evolution of protoplanetary disks: An analytical approach
    Tsukamoto, Yusuke
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2024, 76 (04) : 674 - 687
  • [33] Determining Dust Properties in Protoplanetary Disks: SED-derived Masses and Settling with ALMA
    Rilinger, Anneliese M.
    Espaillat, Catherine C.
    Xin, Zihua
    Ribas, Alvaro
    Macias, Enrique
    Luettgen, Sarah
    ASTROPHYSICAL JOURNAL, 2023, 944 (01):
  • [34] Porous Dust Particles in Protoplanetary Disks: Application to the HL Tau Disk
    Zhang, Shangjia
    Zhu, Zhaohuan
    Ueda, Takahiro
    Kataoka, Akimasa
    Sierra, Anibal
    Carrasco-Gonzalez, Carlos
    Macias, Enrique
    ASTROPHYSICAL JOURNAL, 2023, 953 (01):
  • [35] Dust growth and settling in protoplanetary disks and disk spectral energy distributions. I. Laminar disks
    Tanaka, H
    Himeno, Y
    Ida, S
    ASTROPHYSICAL JOURNAL, 2005, 625 (01): : 414 - 426
  • [36] MILLIMETER-WAVE POLARIZATION OF PROTOPLANETARY DISKS DUE TO DUST SCATTERING
    Kataoka, Akimasa
    Muto, Takayuki
    Momose, Munetake
    Tsukagoshi, Takashi
    Fukagawa, Misato
    Shibai, Hiroshi
    Hanawa, Tomoyuki
    Murakawa, Koji
    Dullemond, Cornelis P.
    ASTROPHYSICAL JOURNAL, 2015, 809 (01):
  • [37] Consistent dust and gas models for protoplanetary disks I. Disk shape, dust settling, opacities, and PAHs
    Woitke, P.
    Min, M.
    Pinte, C.
    Thi, W. -F.
    Kamp, I.
    Rab, C.
    Anthonioz, F.
    Antonellini, S.
    Baldovin-Saavedra, C.
    Carmona, A.
    Dominik, C.
    Dionatos, O.
    Greaves, J.
    Guedel, M.
    Ilee, J. D.
    Liebhart, A.
    Menard, F.
    Rigon, L.
    Waters, L. B. F. M.
    Aresu, G.
    Meijerink, R.
    Spaans, M.
    ASTRONOMY & ASTROPHYSICS, 2016, 586
  • [38] Large dust grains in the inner region of circumstellar disks
    Isella, A
    Testi, L
    Natta, A
    ASTRONOMY & ASTROPHYSICS, 2006, 451 (03) : 951 - 959
  • [39] New Growth Mechanism of Dust Grains in Protoplanetary Disks with Magnetically Driven Disk Winds
    Taki, Tetsuo
    Kuwabara, Koh
    Kobayashi, Hiroshi
    Suzuki, Takeru K.
    ASTROPHYSICAL JOURNAL, 2021, 909 (01):
  • [40] A COMPACT CONCENTRATION OF LARGE GRAINS IN THE HD 142527 PROTOPLANETARY DUST TRAP
    Casassus, Simon
    Wright, Chris M.
    Marino, Sebastian
    Maddison, Sarah T.
    Wootten, Al
    Roman, Pablo
    Perez, Sebastian
    Pinilla, Paola
    Wyatt, Mark
    Moral, Victor
    Menard, Francois
    Christiaens, Valentin
    Cieza, Lucas
    van der Plas, Gerrit
    ASTROPHYSICAL JOURNAL, 2015, 812 (02):
12345