Multiwavelength and Statistical Research in Space Astrophysics

Details Multiwavelength and Statistical Research in Space Astrophysics Multiwavelength and Statistical Research in Space Astrophysics

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nasa.rept.....f&link_type=abstract

Technical Report, NASA-CR-205320; NAS 1.26:205320 Dept.of Astronomy and Astrophysics

Astronomy and Astrophysics

Astrophysics

Active Galactic Nuclei, Astrophysics, X Rays, Radio Galaxies, Bl Lacertae Objects, T Tauri Stars, Protostars, Regression Analysis, Rosat Mission, Radio Observation, Nonthermal Radiation, Radio Emission, Astronomy, Magnetic Variations, Star Formation

Scientific paper

The accomplishments in the following three research areas are summarized: multiwavelength study of active galactic nuclei; magnetic activity of young stellar objects; and statistical methodology for astronomical data analysis. The research is largely based on observations of the ROSAT and ASCA X-ray observatories, complemented by ground-based optical and radio studies. Major findings include: discovery of inverse Compton X-ray emission from radio galaxy lobes; creation of the largest and least biased available sample of BL Lac objects; characterization of X-ray and nonthermal radio emission from T Tauri stars; obtaining an improved census of young stars in a star forming region and modeling the star formation history and kinematics; discovery of X-ray emission from protostars; development of linear regression methods and codes for interpreting astronomical data; and organization of the first cross-disciplinary conferences for astronomers and statisticians.

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