Rudolf Minkowski Jeffrey M. Silverman Astro 290B UC Berkeley 4/25/2006.

Slides:



Advertisements
Similar presentations
3A03 – GR and Cosmology Ralph Pudritz Dept. of Physics & Astronomy McMaster University.
Advertisements

Discoveries in Planetary Sciencehttp://dps.aas.org/education/dpsdisc/ The Discovery Describe an unresolved question or mystery in a given research area,
1 Hydrogen in the Milky Way Hydrogen is the most abundant element in our galaxy. The 21-cm Line.
Recycling in the Universe
Original image: 512 pixels by 512 pixels. Probe is the size of 1 pixel. Picture is sampled at every pixel ( samples taken)
Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Fix Astronomy Chapter 6.
Black Hole in M83 Topic: Black holes Concepts: multi-wavelength observations, black hole evolution Missions: Hubble, Chandra, Swift Coordinated by the.
Exposure: Aperture And Shutter Speed A present to my motivated little photo muffins from your sniffling, coughing teacher For Intermediate- an intro For.
Astro 101 Slide Set: Multiple Views of an Extremely Distant Galaxy 0 Topic: Distant galaxies Concepts: Galaxy development, Gravitational lensing Missions:
July Light pollution map. If interested in astronomy, the last place you want to be is in the Northeast.
Discoveries in Planetary Sciencehttp://dps.aas.org/education/dpsdisc/ A Planet Orbiting Two Suns About 1000 planets have been discovered outside our own.
The Cosmic Simulator Daniel Kasen (UCB & LBNL) Peter Nugent, Rollin Thomas, Julian Borrill & Christina Siegerist.
Edmund Bertschinger MIT Department of Physics and Kavli Institute for Astrophysics and Space Research The Cosmic Menu of Dark Matter and Dark Energy.
How Stars Form Shantanu Basu Physics & Astronomy University of Western Ontario Preview Western, May 3/4, 2003.
Reflectors of the World. The First Reflector First reflector designed by Isaac Newton in 1668.
Light, Mirrors and Telescopes Rajesh Gupta University of California, San Diego. Mr. Smith’s Class.
This is a slide show showing how we grew our vegetables, how the process began and what we got in the end.
A long time ago in a galaxy far, far away
Discoveries in Planetary Sciencehttp://dps.aas.org/education/dpsdisc/ First Rocky Exoplanet Detected Most known exoplanets are large and have low densities.
Shutter Speed.  How long the sensor/film in the camera is being exposed to light  Shutter speed allows light to reach the cameras image sensor  How.
Figure 4 from The Hubble Space Telescope Cluster Supernova Survey. II. The Type Ia Supernova Rate in High-redshift Galaxy Clusters (Image 1 of 3) K. Barbary.
Figure 7 from Effects of Circumnuclear Disk Gas Evolution on the Spin of Central Black Holes (Image 1 of 7) Umberto Maio et al ApJ doi: / X/767/1/37.
Figure 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 1 of 8) A.
Figure 4 from Power Spectrum Analysis of Polarized Emission from the Canadian Galactic Plane Survey (Image 1 of 6) R. A. Stutz et al ApJ doi: / X/787/1/34.
Figure 14 from The Compositional Diversity of Extrasolar Terrestrial Planets. I. In Situ Simulations (Image 1 of 4) Jade C. Bond et al ApJ
Figure 4 from The Australia Telescope Compact Array H I Survey of the Galactic Center (Image 1 of 9) N. M. McClure-Griffiths et al ApJS doi: / /199/1/12.
Figure 15 from Star Formation in the Central 400 pc of the Milky Way: Evidence for a Population of Massive Young Stellar Objects (Image 1 of 2) F. Yusef-Zadeh.
Figure 5 from The Australia Telescope Compact Array H I Survey of the Galactic Center (Image 1 of 5) N. M. McClure-Griffiths et al ApJS doi: / /199/1/12.
Youth AstroNet Program Introduction This presentation based on information and materials from The Harvard-Smithsonian Center for Astrophysics Science Education.
Figure 3 from Multiple Component Outflows in an Active Region Observed with the EUV Imaging Spectrometer on Hinode (Image 1 of 11) P. Bryans et al
K. Decker French et al ApJ doi: / X/801/1/1 Information:
Figure 15 from Cloud–Cloud Collision as a Trigger of the High-mass Star Formation: a Molecular Line Study in RCW120 (Image 1 of 5) K. Torii et al
Figure 7 from The Evolution of Dwarf Galaxy Satellites with Different Dark Matter Density Profiles in the ErisMod Simulations. I. The Early Infalls Mihai.
Figure 5 from The ACS LCID Project. II
What Lies Beyond.
Qing-Wen Tang et al ApJ doi: / X/806/2/194 Information:
Figure 8 from Dust Reddened Quasars in FIRST and UKIDSS: Beyond the Tip of the Iceberg (Image 1 of 5) Eilat Glikman et al ApJ doi: / X/778/2/127.
Youth AstroNet Program Introduction
Vocabulary Station 1. Write the vocabulary word and draw a picture of the word using the Hello Crayon App. Save your picture. 2. Take a photo or video.
Y. Q. Xue et al ApJS doi: / /195/1/10 Information:
A. A. Abdo et al ApJ doi: / X/722/1/520 Information:
Mount Palomar, Mount Wilson, and Lowell Observatory
Gregory D. Fleishman et al ApJ doi: / X/802/2/122 Information:
Figure 5 from The Cool Component and the Dichotomy, Lateral Expansion, and Axial Rotation of Solar X-Ray Jets (Image 1 of 2) Ronald L. Moore et al
Figure 3 from The Cool Component and the Dichotomy, Lateral Expansion, and Axial Rotation of Solar X-Ray Jets (Image 1 of 2) Ronald L. Moore et al
By: David Bouley and Chris Brown
Figure 1 from Toward Precision Photometry for the ELT Era: The Double Subgiant Branch of NGC 1851 Observed with the Gemini/GeMS MCAO System P. Turri et.
Figure 3 from The ACS Nearby Galaxy Survey Treasury. VIII
Figure 3.1 from Witnessing the Differential Evolution of Disk Galaxies in Luminosity and Size via Gravitational Lensing (Image 1 of 5) Kaushala Bandara.
Figure 2 from An X-ray Imaging Survey of Quasar Jets: Testing the Inverse Compton Model (Image 1 of 4) H. L. Marshall et al ApJS doi: / /193/1/15.
Figure 4 from Spectroscopic Properties of Star-forming Host Galaxies and Type Ia Supernova Hubble Residuals in a nearly Unbiased Sample Chris B. D'Andrea.
Figure 1 from Spectroscopic Properties of Star-forming Host Galaxies and Type Ia Supernova Hubble Residuals in a nearly Unbiased Sample Chris B. D'Andrea.
Multiwavelength Astronomy:
Figure 5 from Circumstellar 12C/13C Isotope Ratios from Millimeter Observations of CN and CO: Mixing in Carbon- and Oxygen-Rich Stars (Image 1 of 18) S.
Danielle A. Berg et al ApJ doi: / X/754/2/98 Information:
Catherine Walsh et al ApJ doi: / X/722/2/1607 Information:
Figure 15 from The Carnegie-Irvine Galaxy Survey. II
Figure 3 from Spectral Line Survey toward the Spiral Arm of M51 in the 3 and 2 mm Bands (Image 1 of 6) Yoshimasa Watanabe et al ApJ doi: / X/788/1/4.
Figure 1 from Hubble Space Telescope Combined Strong and Weak Lensing Analysis of the CLASH Sample: Mass and Magnification Models and Systematic Uncertainties.
Figure 3 from Ultraviolet Light Curves of Supernovae with the Swift Ultraviolet/Optical Telescope (Image 1 of 25) Peter J. Brown et al AJ
Figure 2 from High-Resolution Submillimeter Multiline Observations of G19.61 – 0.23: Small-Scale Chemistry (Image 1 of 2) Sheng-Li Qin et al ApJ.
Figure 17 from The SCUBA-2 Cosmology Legacy Survey: Multiwavelength Counterparts to 103 Submillimeter Galaxies in the UKIDSS-UDS Field (Image 1 of 7) Chian-Chou.
Figure 2 from Thermodynamics of the Solar Corona and Evolution of the Solar Magnetic Field as Inferred from the Total Solar Eclipse Observations of 2010.
Figure from Validating Time-Distance Helioseismology with Realistic Quiet-Sun Simulations (Image 1 of 9) K. DeGrave et al ApJ doi: / X/788/2/127.
Figure 6 from Detailed Compositional Analysis of the Heavily Polluted DBZ White Dwarf SDSS J : A Window on Planet Formation? (Image 1.
Tomoharu Oka et al ApJS doi: / /201/2/14 Information:
Figure 2 from Mid-Infrared Properties of OH Megamaser Host Galaxies. I
Shutter SPeed.
Shutter SPeed.
SAND STORM Sand Storm, 26 April Al Asad, IRAQ
Presentation transcript:

Rudolf Minkowski Jeffrey M. Silverman Astro 290B UC Berkeley 4/25/2006

Rudolf Minkowski Picture courtesy of Biographical Memoirs of the National Academy of Science

Rudolf Minkowski Picture courtesy of The Archives of the California Institute of Technology

The Radio Galaxy Cygnus A Taken from the original article by Baade and Minkowski, the image shows a negative of Cygnus A taken at different wavelengths. Photo courtesy of The Astrophysical Journal

Walter Baade Picture courtesy of the Bruce Medalists website:

Palomar 48-inch Schmidt Telescope Picture courtesy of the National Parks Service’s Palomar website:

Palomar 200-inch Hale Telescope Picture courtesy of Wikipedia:

Rudolf Minkowski Picture courtesy of Biographical Memoirs of the National Academy of Science

Minkowski Observing at Palomar: “Where is that thing?...I think that’s it over there…[sound of slow motion motor] Damn! Wrong button [slow motion again]...there it is...now where’s that little double to the left?...no that’s not it...[to the night assistant]…try a little west...stop![to himself]…here it comes…[slow motion]...Ah! Too Much!...[slow motion]...Now I've got it [sound of dark slide opening; then, to the night assistant]…Start the exposure! I'll take three hours on this one. You can rest a while.” This is followed by a long sigh, then he began to hum “Ode to Joy” from Beethoven's Ninth Symphony.

References: Osterbrock, Donald E., Biographical Memoirs of the National Academy of Science, 54, , Plicht, Chris, Rudolph Minkowski,. Robinson, I., et al, 1965, Quasi-Stellar Sources and Gravitational Collapse, Chicago, University of Chicago Press. Tenn, Joseph S., The Bruce Medalists: Rudolph Minkowski, 2004,.

The End ©2006 Cheap Guy Inc.