Analysis of the nebulosities near T Tauri using digital computer image processing

Details Analysis of the nebulosities near T Tauri using digital computer image processing Analysis of the nebulosities near T Tauri using digital computer image processing

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...202..696l&link_type=abstract

Astrophysical Journal, vol. 202, Dec. 15, 1975, pt. 1, p. 696, 697, 699 (12 ff.).

Astronomy and Astrophysics

Astrophysics

11

Imaging Techniques, Luminous Intensity, Nebulae, T Tauri Stars, Digital Computers, Main Sequence Stars, Optical Data Processing, Photography, Radiography, Stellar Luminosity, Wave Reflection

Scientific paper

Direct plates of T Tauri taken with the 120-inch (3 m) and 36-inch (91 cm) Lick reflectors were digitized and analyzed using digital-computer image-processing techniques. Luminous emission protrusions extending to as far as 13-sec from T Tauri in position angles 170 deg, 210 deg, and 330 deg are shown. These features are variable and may contain a layered structure. The complex reflection nebula west of T Tauri (NGC 1555) appears to be an illuminated portion of a much larger dark nebula whose variability is due to obscuring material near the star.

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