The Asymmetric Thermal Emission of the Protoplanetary Disk Surrounding HD 142527 Seen by Subaru/COMICS
暂无分享,去创建一个
Shigeyuki Sako | Takashi Onaka | Takashi Miyata | Hirokazu Kataza | Yoshiko K. Okamoto | Itsuki Sakon | Mitsuhiko Honda | Takuya Yamashita | Misato Fukagawa | Hideaki Fujiwara | Takuya Fujiyoshi
[1] Shigeyuki Sako,et al. Improved performances and capabilities of the Cooled Mid-Infrared Camera and Spectrometer (COMICS) for the Subaru Telescope , 2003, SPIE Astronomical Telescopes + Instrumentation.
[2] C. Dullemond,et al. Correlation between grain growth and disk geometry in Herbig Ae/Be systems , 2004, astro-ph/0404553.
[3] S. Price,et al. A Uniform Database of 2.4-45.4 Micron Spectra from the Infrared Space Observatory Short Wavelength Spectrometer , 2003 .
[4] W. C. Danchi,et al. Imaging the Disk around the Luminous Young Star LkHα 101 with Infrared Interferometry , 2002 .
[5] S. Lord. A new software tool for computing Earth's atmospheric transmission of near- and far-infrared radiation , 1992 .
[6] H. Kataza,et al. Improvements in Operating the Raytheon 320 × 240 Pixel Si:As Impurity Band Conduction Mid‐Infrared Array , 2003 .
[7] M. Min,et al. The building blocks of planets within the ‘terrestrial’ region of protoplanetary disks , 2004, Nature.
[8] M. Min,et al. A 10 μm spectroscopic survey of Herbig Ae star disks: Grain growth and crystallization , 2005, astro-ph/0503507.
[9] Shigeyuki Sako,et al. COMICS: the cooled mid-infrared camera and spectrometer for the Subaru telescope , 2000, Astronomical Telescopes and Instrumentation.
[10] Saeko S. Hayashi,et al. Near-Infrared Images of Protoplanetary Disk Surrounding HD 142527 , 2006 .
[11] Ari Laor,et al. Spectroscopic constraints on the properties of dust in active galactic nuclei , 1993 .
[12] Mark R. Kidger,et al. Spectral Irradiance Calibration in the Infrared. X. A Self-Consistent Radiometric All-Sky Network of Absolutely Calibrated Stellar Spectra , 1999 .
[13] Sebastiano Ligori,et al. Mid-infrared sizes of circumstellar disks around Herbig Ae/Be stars measured with MIDI on the VLTI , 2004 .