VLTI/VINCI observations of the nucleus of NGC 1068 using the adaptive optics system MACAO
暂无分享,去创建一个
[1] G. Perrin,et al. A catalogue of calibrator stars for long baseline stellar interferometry , 2002 .
[2] Bonn,et al. From the Circumnuclear Disk in the Galactic Center to thick, obscuring tori of AGNs , 2003, astro-ph/0310329.
[3] 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 .
[4] L. Danese,et al. Thick tori around active galactic nuclei: a comparison of model predictions with observations of the infrared continuum and silicate features , 1994 .
[5] Martin J. Ward,et al. The polarization of NGC 1068. , 1988 .
[6] Bonn,et al. Where have all the black holes gone , 2002, astro-ph/0203489.
[7] Karl-Heinz Hofmann,et al. Interferometric studies of nearby galactic centers , 2003, SPIE Astronomical Telescopes + Instrumentation.
[8] M. Rowan-Robinson,et al. Dusty discs in active galactic nuclei , 1995 .
[9] J. Bland-Hawthorn,et al. The Ringberg Standards for NGC 1068 , 1997 .
[10] R. Barvainis,et al. Hot Dust and the Near-Infrared Bump in the Continuum Spectra of Quasars and Active Galactic Nuclei , 1987 .
[11] Andreas Quirrenbach,et al. The Nuclear Stellar Core, the Hot Dust Source, and the Location of the Nucleus of NGC 1068 , 1997 .
[12] Robert Antonucci,et al. Unified models for active galactic nuclei and quasars , 1993 .
[13] Rainer Wilhelm,et al. VINCI, the VLTI commissioning instrument: status after one year of operations at Paranal , 2003, SPIE Astronomical Telescopes + Instrumentation.
[14] D. Segransan,et al. Data reduction methods for single-mode optical interferometry Application to the VLTI two-telescopes beam combiner VINCI , 2004 .
[15] Z. Ivezic,et al. Dust Emission from Active Galactic Nuclei , 2002 .
[16] Thierry Forveille,et al. High angular resolution K-band spectroscopy of the nucleus of NGC 1068 with PUEO-GRIF (CFHT) , 2003 .
[17] Julian H. Krolik,et al. Infrared spectra of obscuring dust tori around active galactic nuclei. I - Calculational method and basic trends , 1992 .
[18] J. Miller,et al. Spectropolarimetry and the nature of NGC 1068 , 1985 .
[19] Julian H. Krolik,et al. Molecular tori in Seyfert galaxies - Feeding the monster and hiding it , 1988 .
[20] Gerd Weigelt,et al. Diffraction-limited bispectrum speckle interferometry of the nuclear region of the Seyfert galaxy NGC 1068 in the H and K' bands , 2004 .
[21] M. Dopita,et al. Probing the Dusty Accretion Torus of Seyfert Galaxies , 1998 .
[22] G. Neugebauer,et al. Diffraction-limited Imaging and Photometry of NGC 1068 , 1999 .
[23] B. Krauskopf,et al. Proc of SPIE , 2003 .
[24] M.Swain,et al. Interferometer Observations of Subparsec-Scale Infrared Emission in the Nucleus of NGC 4151 , 2003 .
[25] Andreas Glindemann,et al. VINCI: the VLT Interferometer commissioning instrument , 2000, Astronomical Telescopes and Instrumentation.
[26] J. J. Bock,et al. Draft version : ( ) document High Spatial Resolution Imaging of NGC 1068 in the Mid Infrared , 2022 .