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Bibliography for R. Brent Tully: 1972-present [1] Inclination Corrections to the Optical Luminosities and Diameters of Galaxies. 1972. Tully, R.B. Mon.Not. R.Ast.Soc., 159: 35P-40P. [2] The Kinematics and Dynamics of M51. 1972. Tully, R.B. Ph.D. Thes -
Normal Galaxies in the Local Universe Published in "Astrophysics with Infrared Surveys: A Prelude to SIRTF", 1999. NORMAL GALAXIES IN THE LOCAL UNIVERSE G. Helou SIRTF Science Center, California Institute of Technology, Pasadena, CA 91125 Abstract -
Vol 457j1 January 2009jdoi:10.1038/nature07621 REVIEWS 18 years of science with the Hubble Space Telescope Julianne J. Dalcanton1,2 After several decades of planning, the Hubble Space Telescope (HST) was launched in 1990 as the first of NASAs Great -
SCUBA2: The next generation submillimetre camera for the James Clerk Maxwell Telescope Boulder Outline The SCUBA revolution Why do we need a next generation SCUBA? Comparison of SCUBA2 with other instruments Case studies Specific science example -
Galactic Structure Lecture #2 Paul Woodward 4/16/03 1 Radio observations of atomic H and molecular clouds reveal asymmetry of our galaxy. Gas density not same as you go around in circle at one radius. Spiral arms give slight wiggles in rotation cur -
Galactic Structure Lecture #2 Paul Woodward 4/16/03 Radio observations of atomic H and molecular clouds reveal asymmetry of our galaxy. Gas density not same as you go around in circle at one radius. Spiral arms give slight wiggles in rotation curve. -
Galactic Structure Lecture #2 Paul Woodward 4/16/03 Perseus Arm Orion Arm (spur?) Rotation Sun Optical features Concentrated radio features ? General neutral hydrogen (radio > 1 atom/cm3) + Center Sagitarius Arm Fig. 20.11 Centaurus Arm Parsecs -
Chapter 16 Galaxies II Lecture 25 19 April 2007 Galaxies Star systems like our Milky Way Contain a few thousand to tens of billions of stars. Large variety of shapes and sizes Galaxy Diversity Even seemingly empty regions of the sky contain tho -
EXTRASOLAR ANALOGUES TO THE KUIPER BELT MARK C. WYATT, WAYNE S. HOLLAND, JANE S. GREAVES and WILLIAM R. F. DENT UK Astronomy Technology Centre Abstract. Debris disks are found around some 15% of main sequence stars and their dust is thought to be co -
Galactic Structure Lecture #2 Paul Woodward 11/27/07 Radio observations of atomic H and molecular clouds reveal asymmetry of our galaxy. Gas density not same as you go around in circle at one radius. Spiral arms give slight wiggles in rotation curve -
Galactic Structure Lecture #2 Paul Woodward 11/27/07 1 Radio observations of atomic H and molecular clouds reveal asymmetry of our galaxy. Gas density not same as you go around in circle at one radius. Spiral arms give slight wiggles in rotation cu -
Astro 6590: Galaxies and the Universe Lecture #2 (Wed Sep 3, 2008) Extinction and reddening Overview of stars Star counts Luminosity functions Malmquist bias Overview of the H-R diagram Color magnitude diagrams (CMDs) Overview of stellar evol -
Chapter Summary The Historical Problem of the "Nebulae" This lecture is based on the following reading in your text: Chapter 21. Galaxies The topics in this lecture are: The Historical Problem of the "Nebulae" The Morphology of Gala -
REFERENCES FOR THE CATALOGUE 1. AARONSON M., HUCHRA J., MOULD J. R., 1979. ASTROPHYS. J., 229, 1. 2. AARONSON M., MOULD J. R., HUCHRA J., 1980. ASTROPHYS. J., 237, 655. 3. AARONSON M., DAWE J. A., DICKENS R. J., MOULD J. R., -
Dust particles and their spectra. Summary. Here are the articles and reviews I read in preparation of the final report. Review at http:/nedwww.ipac.caltech.edu/level5/Sept03/Li/Li1.html "Hot Very Small dust Grains in NGC 1068 seen in jet induced