Nashville Is…
Find out why Nashville is one of the best cities in the country to live.
VUCast: Celebrate, celebrate…amazing seniors
Meet several impressive Vanderbilt graduates who took their bold ideas outside of the classroom. Plus, high tech changes are coming to the Commencement ceremony and hear from the real life “Mother Earth.”
VUCast Extra: Be Agents of Change!
Nobel Prize winner, Green Belt Movement founder, and this year’s recipient of the Nichols-Chancellor’s medal Wangari Maathai gave students an inspirational call to action at Senior Day. Hear from Maathai and the graduates. Read more >>
Senior Day Speaker Wangari Maathai
Watch video of Wangari Maathai, the 2004 recipient of the Nobel Peace Prize and founder of the environmentally conscious Green Belt Movement, receiving Vanderbilt University’s prestigious Nichols-Chancellor’s Medal May 12 during Senior Day. The Nichols-Chancellor’s Medal, which includes a cash prize, is one of the university’s highest honors and is given to individuals who define thekeep reading »
Commencement 2011
Watch video of Vanderbilt University’s class of 2011 Commencement ceremony. About 2,843 graduates were expected to attend Commencement. Degrees were scheduled to be awarded to 1,734 undergraduate and 1,904 graduate students. The main ceremony, featuring the annual address to graduates from Chancellor Zeppos, was moved to Memorial Gym due to the weather. After Chancellor Zepposkeep reading »
8.7 Luminosity functions
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
8.6 Line spectra: Activity 8 Quasar redshifts
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
8.5 Line spectra: Activity 7 Colours and broad lines
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
8.4 Line spectra: line flux and equivalent width
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
8.3 Line spectra: ions and spectral lines
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
8.2 Extended radio sources
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
8.1 Continuum spectra
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
7.9 Compton scattering
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
7.8 Example 2 and questions
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
7.7 Radiation detection
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
7.6 Producing synchroton radiation in a laboratory
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
7.5 Emission from spiralling electrons: synchrotron radiation
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
7.4 Faraday depolarization
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
7.3 Polarization of electromagnetic radiation
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
7.2 Free-free radiation
Active galaxies provide a prime example of high energy processes operating in the Universe. This unit gives an overview of active galaxies, including the supermassive black holes that power the engines at their centres, and the emission processes by which we detect and study them. It also gives practice in mathematical techniques for analysing data and theoretical models.
