21. UC Santa Barbara Astrophysics Home Page The UC Santa Barbara astrophysics Project. WELCOME. to our astrophysics Web site at the Physics department of UCSB http://www.deepspace.ucsb.edu/

The UC Santa Barbara Astrophysics Project W ELCOME to our Astrophysics Web site at the Physics department of UCSB. Comet Hyakutake March 8, 1996 UCSB ROT 30s. Image Unfiltered UCSB Astro Research Learn about Astrophysics research efforts at UCSB RAAP Telescope Connect to the Remotely Operated Telescope (ROT) and to the Remote Access Astronomy Project (RAAP) Interactive Astrophysics The doors of perception to the Universe are opened here, for you. Images Stroll through our database of heavenly images. Utilities Download the software neccesary to decompress and view our images. Triffid Nebula Other Topics CONTRIBUTORS ABOUT UCSB WWW SERVERS Please address questions or comments to Last Modified: January 21, 2004

22. SpringerLink - Publication A service of the Laboratory for High Energy astrophysics (LHEA) at NASA/ GSFC and the High Energy astrophysics Division of the Smithsonian Astrophysical http://link.springer.de/link/service/journals/00230/&e=747

Articles Publications Publishers Home Publication Astronomy and Astrophysics Publisher: Springer-Verlag Heidelberg ISSN: 0004-6361 (Paper) 1432-0746 (Online) Subject: Geosciences Physics and Astronomy This journal is hosted on another site at: Astronomy and Astrophysics Publication 1 of 1 Previous Publication Next Publication Linking Options Table Of Contents Alerting Click the button below to enable Table Of Contents Alerting for this publication. For assistance inside the Americas: springerlink@springer-ny.com , For assistance outside the Americas: springerlink@springer.de HTTP User Agent: SecretBrowser/007

23. VUW | SCPS - School Of Chemical And Physical Sciences The Microlensing Observations in astrophysics (MOA) Project is a joint Japanese/New Zealand experiment established in 1995 to carry out astrophysical observations from New Zealand using `gravitational microlensing' and related techniques. http://www.vuw.ac.nz/scps/moa/

Welcome to SCPS! Course Support Safety Information Employment Opportunities Read all notices PROSPECTIVE STUDENTS UNDERGRADUATE STUDENTS POSTGRADUATE STUDENTS ... CONTRACT SERVICES Glassblowing, Electron Microscopes, Mass Spectrometry Last updated Monday 07 June 2004 Questions or comments to SCPS Web Administrator Read Victoria University

24. Imagine The Universe! Dictionary This site is intended for students age 14 and up, and for anyone interested in learning about our universe. of celestial bodies and phenomena. astrophysics. The part of astronomy that deals principally with the It was previously named the Advanced Xray astrophysics Facility (AXAF). http://imagine.gsfc.nasa.gov/docs/dictionary.html

Imagine the Universe! Dictionary Please allow the whole page to load before you start searching for an entry. Otherwise, errors will occur. A B C D ... Z (Note - Greek letters are written out by name - alpha, beta etc.) A accretion Accumulation of dust and gas onto larger bodies such as stars, planets and moons. accretion disk A relatively flat sheet of gas and dust surrounding a newborn star, a black hole, or any massive object growing in size by attracting material. active galactic nuclei (AGN) A class of galaxies which spew massive amounts of energy from their centers, far more than ordinary galaxies. Many astronomers believe supermassive black holes may lie at the center of these galaxies and power their explosive energy output. Tell me about AGN! Tell me more about AGN! angstrom A unit of length equal to 0.00000001 centimeters. This may also be written as 1 x 10 cm (see scientific notation angular momentum A quantity obtained by multiplying the mass of an orbiting body by its velocity and the radius of its orbit. According to the conservation laws of physics, the angular momentum of any orbiting body must remain constant at all points in the orbit, i.e., it cannot be created or destroyed. If the orbit is elliptical the radius will vary. Since the mass is constant, the velocity changes. Thus planets in elliptical orbits travel faster at perihelion and more slowly at aphelion . A spinning body also possesses spin angular momentum. apastron The point of greatest separation between two stars which are in orbit around each other. See

25. WebStars Astrophysics In Cyberspace WebStars astrophysics in Cyberspace. This list of astronomical resource of terms. History of Astronomy and astrophysics. 4000 years of http://heasarc.gsfc.nasa.gov/docs/outreach/webstars.html&e=747

26. NAP2001 - Nuclear Astrophysics 2001 The symposium, which is organized in celebration of KarlLudwig Kratz, Claus Rolfs and Friedrich-Karl Thielemann, aims to cover the most exciting and important developments in nuclear astro- physics by a series of invited talks. http://nap2001.gsi.de/

27. Oxford Astrophysics OXFORD astrophysics. FOR VISITORS About Us How to Find Us JOBS Jobs and Research Positions GRADUATE STUDIES Information for Prospective http://www-astro.physics.ox.ac.uk/&e=747

28. Science Education Department -- Harvard-Smithsonian Develops curricula, videos and activities to enhance learning of scientific topics. Includes list of projects and staff. http://cfa-www.harvard.edu/cfa/sed/

T SED research and materials are widely available through print and CD-ROM, on the Internet and television, by teleconferencing, and at workshops and teacher conferences. Through its efforts, the SED aims to advance the public's understanding of astronomy and the physical sciences. Support for SED projects comes from the National Science Foundation, the Annenberg/CPB Projects, NASA, the Department of Commerce, and others. Additional support is provided by the Smithsonian Institution, Harvard College Observatory, and the Harvard University Graduate School of Education. Projects People Resources View SED-produced programming on-demand, on broadband, at the Annenberg/CPB Channel site . Online video includes recent teacher professional development workshops: Private Universe Project in Math Science in Focus: Energy , and Science in Focus: Force and Motion Harvard-Smithsonian Center for Astrophysics Science Education Department 60 Garden Street, MS-71; Cambridge, MA 02138

29. NASA ADS: ADS Home Page Free online abstracts and fulltext papers in astronomy, astrophysics, planetary sciences, and solar physics. http://adswww.harvard.edu/

ADS Services Search Browse Mirrors Feedback ... What's new Other NASA Centers CXC HEASARC IRSA LAMBDA ... SPITZER Related Sites AAS ADEC CDS IAU ... Preprints CfA CfA CfA Preprints Chandra Harvard University ... The NASA Astrophysics Data System The Digital Library for Physics, Astrophysics, and Instrumentation This site is hosted by the Harvard-Smithsonian Center for Astrophysics Mirror sites Help Site Map The Astrophysics Data System (ADS) is a NASA-funded project which maintains four bibliographic databases containing more than 3.9 million records: Astronomy and Astrophysics, Instrumentation, Physics and Geophysics, and preprints in Astronomy. The main body of data in the ADS consists of bibliographic records, which are searchable through our Abstract Service query forms , and full-text scans of much of the astronomical literature which can be browsed though our Browse interface For more information, please read our page detailing the Terms and Conditions regulating the use of our resources. In addition to its databases, the ADS provides access and pointers to a wealth of external resources, including electronic articles, data catalogs and archives. We currently have links to over 4.0 million records maintained by our collaborators. The importance of ADS's role in supporting the scientific community has been recognized by societies and individuals . If you wish to acknowledge us in a publication, kindly use a phrase such as the following:

30. Kluwer Academic Publishers - Astrophysics http://www.kluweronline.com/issn/0571-7256/contents&e=747

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31. All About Amazing Astronomy Basic information on astronomy and astrophysics. http://www.astro-india.8m.com

Free Web site hosting - Freeservers.com Web Hosting - GlobalServers.com Choose an ISP NetZero High Speed Internet ... Dial up $14.95 or NetZero Internet Service $9.95 WELCOME TO OUR HOME PAGE!!! This is a good astronomical site. Here you can know a lot of information. You can copy any information from this site.You can also copy pictures by the approval of the owner. VISIT OUR OTHER PAGES FOR "PICS" Adding captions makes my pictures more interesting. Planet details THE SPACE AGE The voyage of space beyond the EARTH has been one of the man's dream for a long time. (KLAW-DEE-UHS TAHL-UH-MEE) 2nd century, which was accepted by scientist as correct for over a thousands of yrs. Favorite links Other links

32. Kluwer Academic Publishers - Astrophysics http://www.kluweronline.com/issn/0571-7256/current&e=747

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33. Faculty Profile: Bernard F. Burke Professor of astrophysics, Massachusetts Institute of Technology. A profile of Bernard Burke and his work in radio astronomy http://rleweb.mit.edu/Publications/currents/4-1facpr.HTM

FACULTY PROFILE: Bernard E Burke Boston native and William A.M. Burden Professor of Astrophysics Bernard R. Burke completed his SB in 1950 and PhD in 1953 at MIT. In 1953, he joined the Department of Terrestrial Magnetism at the Carnegie Institution in Washington and became a section manager in 1957. Upon his return to MIT in 1965 as Professor of Physics, Professor Burke introduced interferometric techniques at the Haystack Radio Observatory in Westford, Massachusetts. As leader of RLE's research group in this area, he shared the 1971 Rumford Prize awarded by the Academy of A rts and Sciences. Together with the National Radio Astronomy Observatory and the Canadian National Research Council, his research group developed techniques for very-long-baseline interferometry (VLBI). This method uses atomic frequency standards to synchronize radio teles copes at remote locations around the world and has improved angular resolution for radio telescopes by 1000-fold. Professor Burke's group was also first to conduct inter- and transcontinental VLBI. Recently, he has served as the U.S. principal investigato r to develop orbiting VLBI stations and has also participated in European and Soviet VLBI mission studies. He has served as Visiting Professor at the University of Leiden (1971-72), Sherman Fairchild Scholar at the California Institute of Technology (1984- 85), and held a Smithsonian Regents Fellowship in 1985. In 1963, he received the Warner Prize of the Amer ican Astronomical Society and, in 1988, was corecipient of a NASA Group Achievement Award. He served as President of the American Astronomical Society (1986-88), is Fellow of the American Academy of Arts and Sciences, and was elected to the National Acade my of Sciences in 1970. He chairs and serves on several advisory boards for NASA and the National Science Foundation, and participates on the editorial boards of many professional journals.

34. RSSD - Research Science Home Page ESA Home, Research Science Home, SciTech Portal. astrophysics, Planetary Exploration, Solar Terrestrial Science, Fundamental Physics, Science Operations, Research. http://www.rssd.esa.int/&e=747

35. Laser Star Astrophysics Plasma recombination lasers in rapidly cooled stellar atmospheres (plasma laser astrophysics) including history of the laser and astronomical spectroscopy. http://www.achilles.net/~jtalbot/index.html

36. University Of Chicago Department Of Astronomy Astrophysics UChicago webmaster@astro.uchicago.edu 5640 S. Ellis Ave, Chicago, IL 60637 773702-8203 Colloquia and Seminars Department Resources. Yerkes Observatory. http://astro.uchicago.edu/&e=747

37. SAO Telescope Data Center Creates, and maintains software to process and archive data from optical telescopes at the Oak Ridge Observatory in Harvard, Massachusetts, Whipple Observatory, and Multiple Mirror Telescope on Mt. Hopkins in Arizona. The Smithsonian Astrophysical Observatory (SAO) is part of the Harvard Smithsonian Center for astrophysics (CfA) in Cambridge, Massachusetts. http://cfa165.harvard.edu/

Harvard-Smithsonian Center for Astrophysics The SAO Telescope Data Center in Cambridge, Massachusetts , supports proposing scheduling observing computing , data reducing and analyzing, and data archiving for these optical telescopes Telescopes and Instruments ... Oak Ridge Observatory in Harvard, Massachusetts Whipple Observatory on Mt. Hopkins in Arizona. 48" schedule 60" schedule (Quarterly Report) (Email for Problems) ... MMT Observatory on Mt. Hopkins in Arizona. MMT schedule Time Allocation Committee ... skymap Making Charts from Astronomical Catalogs (Making Images) Software: widl Making Finding Charts from DSS Images Data svdfit Removing sky from spectra ApJ Letters paper Reduction stelircam Reducing Stelircam output Software hectospec Reducing Hectospec output Data rvsao Computing Redshifts in IRAF papers Analysis SAOimage Displaying Images papers Software: WCSTools Using Sky Coordinates in Astronomical Images papers Image header manipulation utilities Results Updated Zwicky Catalog of Galaxies CfA Redshift Survey Large Scale Structure Galaxy and Cluster LX-sigma Relation ... Spectra of Supernovae Resources Spectrograph Archives [Z-Machine] [FAST] [UZC(both)] ... Mt. Hopkins Interactive Tour

38. NRC-HIA Web Site Has Moved / Site Web De L'IHA-CNRC A Déménagé NRC Herzberg Institute of astrophysics Expertise that delivers across the entire spectrum. http://www.hia.nrc.ca/&e=747

NRC-HIA Web Site Has Moved hia.nrc.gc.ca Due to this move and the restructuring of our site, old bookmarks will need to be updated. Sorry for the inconvenience. iha.cnrc.gc.ca

39. Download Files BRUCE and KYLIE are Fortran 77 codes by Rich Townsend which calculate synthetic spectra for stars undergoing nonradial pulsation (NRP). TLUSTY and SYNSPEC are Fortran 77 codes by Ivan Hubeny and Thierry Lanz for calculating synthetic plane-parallel stellar atmospheres and associated spectra, respectively. http://www.star.ucl.ac.uk/~rhdt/download/

Download Files Home Page Overview This page offers downloads for both codes that I have written, and data which accompanies scientific papers which I have written. The following downloads are on offer: Source code for the BRUCE / KYLIE pulsation modeling codes Source code for the Fortran 95 module , which provides a varying-length string data type conformant to the API specified in ISO/IEC 1539-2:2000 Patches to enable the TLUSTY / SYNSPEC model atmosphere codes to be compiled using the GNU g77 compiler Data to accompany the scientific paper ` Photometric modeling of slowly-pulsating B stars ' (MNRAS, 330, 855) Animations to accompany the scientific paper ` Interactions between Rotation and Pulsation ' (Proc. IAU Symposium 215) BRUCE / KYLIE BRUCE and KYLIE are state-of-the-art FORTRAN 77 codes which calculate synthetic spectra for stars undergoing non-radial pulsation (NRP). These codes are freely distributed, in open-source format, under the GNU General Public License . The source may be downloaded using one of the following links (all files are in UNIX .tar.gz format). File Date Comments bruce-2.84-3.tar.gz

40. AAVSO Hands-On Astrophysics Home Page HandsOn astrophysics, an educational project of the AAVSO, is an invitation to embark upon a journey into the very hearts of starsto listen to and observe http://hoa.aavso.org/&e=747

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