Spiral Structure in the Circumstellar Disk around AB Aurigae
By M. Fukagawa, M. Hayashi, Motohide Tamura, Y. Itoh, S. Hayashi, Y. Oasa, T. Takeuchi, J. Morino, K. Murakawa, S. Oya and 13 more. 2004
175 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/bfd706828ef421f2d7baf5f9621da7f9955bc3d3
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In Astronomy and Astrophysics
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Citations in the corpus
- Dust Growth and Settling in Protoplanetary Disks and Disk Spectral Energy Distributions. I. Laminar Disks (2005, background): “Recent observations with high resolution at various wavelengths gave us much information on disk spatial structure (e.g., Grady et al. 1999; Fukagawa et al. 2004; Mundy et al. 1996; Kitamura et al. 2002; Eisner et al. 2003).”
- Evidence for a co-moving sub-stellar companion of GQ Lup (2005, unknown): “We use 21.33 ± 0.02 mas/pixel as CIAO pixel scale (Fukagawa et al. 2003, 2004) and 45.545 ± 0.005 mas/pixel for HST/PC (Holtzman et al. 1995).”
- Protoplanetary Disks and Their Evolution (2011, background): “Optical and near-infrared coronagraphic imaging by Grady et al. (1999) and Fukagawa et al. (2004) show spiral features in scattered light.”
- The shape of the inner rim in proto-planetary disks (2005, background): “6 includes some rather face-on objects such as AB Aur (LNIR/L⋆ ∼ 0.20, i ∼ 20◦ − 40◦; Fukagawa et al. 2004) and HD 163296 (LNIR/L⋆ ∼ 0.21, i ∼ 30◦; Grady et al. 2000) and some UXORS variable, such as UX Ori, WW Vul and CQ Tau, which are generally considered to be close to edge-on, and have values…”
- DIRECT IMAGING OF FINE STRUCTURES IN GIANT PLANET-FORMING REGIONS OF THE PROTOPLANETARY DISK AROUND AB AURIGAE (2011, background): “We consider the ellipse shape to be due to inclination (Lagage et al. 2006); the southeast side of the ring is inclined toward us (Fukagawa et al. 2004).”
- Sub-arcsec imaging of the AB Aur molecular disk and envelope at millimeter wavelengths: a non Keplerian disk (2005, methodology): “First, the sub-arcsecond image of the continuum emission at 1.4 mm extends inwards the spiral structure detected in the near IR by Fukagawa et al. (2004).”
- The Burst Mode of Protostellar Accretion (2006, background): “Strong observational evidence for the existence of spiral structure in the several-million-year-old disks around AB Aurigae (Fukagawa et al. 2004) and HD 100546 (Grady et al. 2001) tend to support this conjecture.”