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Itinerary As Printable PDF
... Alexander Murrell has taught Astronomy and Physics for 25 years at Wynstones Rudolf Steiner School and is interested in all aspects of cosmology from ancient to modern. ...
... Alexander Murrell has taught Astronomy and Physics for 25 years at Wynstones Rudolf Steiner School and is interested in all aspects of cosmology from ancient to modern. ...
CV - iucaa
... • Kaplan, D. L., van Kerkwijk, M., Bhalerao, V., et al. The Strange Metal-Rich Companion to the Eclipsing Millisecond Pulsar PSR J1816+4510. In American Astronomical Society Meeting Abstracts, volume 221 of American Astronomical Society Meeting Abstracts, page #412.05. 2013. • Miyasaka, H., HongJun, ...
... • Kaplan, D. L., van Kerkwijk, M., Bhalerao, V., et al. The Strange Metal-Rich Companion to the Eclipsing Millisecond Pulsar PSR J1816+4510. In American Astronomical Society Meeting Abstracts, volume 221 of American Astronomical Society Meeting Abstracts, page #412.05. 2013. • Miyasaka, H., HongJun, ...
here - Wellington Astronomical Society
... Meetings usually host a guest speaker, and talks assume that the audience has little or no knowledge of the topic. Afterwards, people can stay for a light supper and often learn from or help others with similar interests. A short meeting of members who are interested in Research Astronomy is held at ...
... Meetings usually host a guest speaker, and talks assume that the audience has little or no knowledge of the topic. Afterwards, people can stay for a light supper and often learn from or help others with similar interests. A short meeting of members who are interested in Research Astronomy is held at ...
The age–metallicity distribution of earth-harbouring stars
... result confirms that younger stars are, on average, more metalrich than older stars. There is a very small scatter around a mean relation, although the number of stars formed at different epochs is not constant. ...
... result confirms that younger stars are, on average, more metalrich than older stars. There is a very small scatter around a mean relation, although the number of stars formed at different epochs is not constant. ...
From eclipse drawings to the coronagraph and spectroscopy
... green line: Fe XIV (530.3 nm) yellow line: Ca XV (569.4 nm) red line: ...
... green line: Fe XIV (530.3 nm) yellow line: Ca XV (569.4 nm) red line: ...
proposed research projects for pparc gemini studentships
... properties (masses and dynamics). GEMINI spectroscopy will allow us to measure kinematics and line strengths out to large radii. We will combine this information with available HST photometry and analyse it using detailed dynamical and stellar population models. Existing data already hint at interes ...
... properties (masses and dynamics). GEMINI spectroscopy will allow us to measure kinematics and line strengths out to large radii. We will combine this information with available HST photometry and analyse it using detailed dynamical and stellar population models. Existing data already hint at interes ...
Discovery of Eclipsing Binary with the Longest Known Period
... although they were in emission during eclipse. The emission components of the lines may possibly also be present, but their intensities are near noise level due to the very strong spectrum of the red giant. Following the MASTER discovery announcement, the new variable star was added to AAVSO interna ...
... although they were in emission during eclipse. The emission components of the lines may possibly also be present, but their intensities are near noise level due to the very strong spectrum of the red giant. Following the MASTER discovery announcement, the new variable star was added to AAVSO interna ...
First generation stars
... Galaxies Speaker: Michael Loewenstein Institute: Astrophysics Science Division, NASA/Goddard Space Flight Center, USA Time: 4:00 pm, 27 May 2010,ThursdayVenue: seminar room, KIAA, Peking University ...
... Galaxies Speaker: Michael Loewenstein Institute: Astrophysics Science Division, NASA/Goddard Space Flight Center, USA Time: 4:00 pm, 27 May 2010,ThursdayVenue: seminar room, KIAA, Peking University ...
The Search for New “r-process-Enhanced” Metal
... • Astronomers need to “fill out the phase space” of variations in r-process enhanced stars • This requires discovery of as many additional examples of the phenomenon as possible • A dedicated survey effort is underway, making use of the world’s largest telescopes • However, they are VERY rare - 3% o ...
... • Astronomers need to “fill out the phase space” of variations in r-process enhanced stars • This requires discovery of as many additional examples of the phenomenon as possible • A dedicated survey effort is underway, making use of the world’s largest telescopes • However, they are VERY rare - 3% o ...
Discovery of Neptune`s Ring at La Silla
... astronomical observations. Using high-speed photometrie techniques the intensity ofthe star light is measured during the passage of the rings through the line of sight which dims the intensity in the order of a few seconds. Such occultations by, and appulses to, interesting planets are predicted and ...
... astronomical observations. Using high-speed photometrie techniques the intensity ofthe star light is measured during the passage of the rings through the line of sight which dims the intensity in the order of a few seconds. Such occultations by, and appulses to, interesting planets are predicted and ...
India-UK strike new solar, nano tech pacts
... "The UK is among the most important countries where we have a very dynamic engagement. In India, we are taking up renewable energy in a big way, and in the solar area we will have an even more active engagement with the UK now," he told reporters at the Indian High Commission today. Describing his U ...
... "The UK is among the most important countries where we have a very dynamic engagement. In India, we are taking up renewable energy in a big way, and in the solar area we will have an even more active engagement with the UK now," he told reporters at the Indian High Commission today. Describing his U ...
Word - QMUL physics
... method for measuring the temperature at formation of the lunar globules. Dr. Batchelder completed his leave in the U.S.A. as Visiting Associate Professor at the University of Delaware for July and August. We welcomed Dr. V. N. Murzin from Moscow for six weeks in October/November to collaborate with ...
... method for measuring the temperature at formation of the lunar globules. Dr. Batchelder completed his leave in the U.S.A. as Visiting Associate Professor at the University of Delaware for July and August. We welcomed Dr. V. N. Murzin from Moscow for six weeks in October/November to collaborate with ...
PowerPoint file - National Optical Astronomy Observatory
... Imager (MDI) instrument aboard the SOHO spacecraft have jointly accumulated more than five years of helioseismic data, with nearly four years of contemporaneous observations. The results from the two projects are generally in good agreement; however, there are differences in detail which need to be ...
... Imager (MDI) instrument aboard the SOHO spacecraft have jointly accumulated more than five years of helioseismic data, with nearly four years of contemporaneous observations. The results from the two projects are generally in good agreement; however, there are differences in detail which need to be ...
WASP-5b: a dense, very hot Jupiter transiting a 12th
... an e2v 2k × 2k CCD, covering 7.8◦ × 7.8◦ . WASP-South started operating in 2006 May with a strategy of tiling up to eight pointings with a cadence of 5–10 min, taking two 30-s exposures at each pointing. The WASP hardware, observing strategy, data reduction pipeline and archive are described in deta ...
... an e2v 2k × 2k CCD, covering 7.8◦ × 7.8◦ . WASP-South started operating in 2006 May with a strategy of tiling up to eight pointings with a cadence of 5–10 min, taking two 30-s exposures at each pointing. The WASP hardware, observing strategy, data reduction pipeline and archive are described in deta ...
WASP-5b: a dense, very hot Jupiter transiting a 12th
... Transit searches are most sensitive to large, Jupiter-sized planets in very short orbits. WASP-5b, like the recently announced WASP3b and WASP-4b, has an ultrashort period below 2 d (Pollacco et al. 2008; Wilson et al. 2008). We discuss the characteristics of these ultraclose, highly irradiated plan ...
... Transit searches are most sensitive to large, Jupiter-sized planets in very short orbits. WASP-5b, like the recently announced WASP3b and WASP-4b, has an ultrashort period below 2 d (Pollacco et al. 2008; Wilson et al. 2008). We discuss the characteristics of these ultraclose, highly irradiated plan ...
Nature template - PC Word 97
... linear distance of ~2 light-years ~ 21018 cm between the end of the ACZ and the core at 7 mm wavelength. The flatness of the radio spectrum down to ~0.7 mm wavelength20 implies that the jet is a self-similar cone with constant Lorentz factor downstream of the point where the jet cross-section becom ...
... linear distance of ~2 light-years ~ 21018 cm between the end of the ACZ and the core at 7 mm wavelength. The flatness of the radio spectrum down to ~0.7 mm wavelength20 implies that the jet is a self-similar cone with constant Lorentz factor downstream of the point where the jet cross-section becom ...
幻灯片 1 - Institute of Astronomy, Cambridge
... The 28th General Assembly of the International Astronomical Union (IAU/GA) was awarded to China for the first time, and will be held in 2012. NAOC will be in charge of organizing. The historical milestone would undoubtedly promote the international status and influences of Chinese astronomy, and wou ...
... The 28th General Assembly of the International Astronomical Union (IAU/GA) was awarded to China for the first time, and will be held in 2012. NAOC will be in charge of organizing. The historical milestone would undoubtedly promote the international status and influences of Chinese astronomy, and wou ...
Day-1
... supplemental problems. The math level is basic algebra. If you are interested, see Dr. Buckner to sign up for the class. It may be planetary but much of the material is also applicable for stellar. ASTR 2020 Problems in Stellar is a spring class. ...
... supplemental problems. The math level is basic algebra. If you are interested, see Dr. Buckner to sign up for the class. It may be planetary but much of the material is also applicable for stellar. ASTR 2020 Problems in Stellar is a spring class. ...
PHYSICAL RESEARCH LABORATORY
... 1. Five days (29 July - 02 August 2008) workshop; sponsored by Punjab State Council for Science and Technology & Vigyan Prasar, Noida. 65 physics teachers from all the 20 district of Punjab attended the workshop. 2. Five days (19th-23rd November, 2009) Introductory workshop in Astronomy & Astrophysi ...
... 1. Five days (29 July - 02 August 2008) workshop; sponsored by Punjab State Council for Science and Technology & Vigyan Prasar, Noida. 65 physics teachers from all the 20 district of Punjab attended the workshop. 2. Five days (19th-23rd November, 2009) Introductory workshop in Astronomy & Astrophysi ...
List of Preprints Contents
... fourteen optical telescopes with diameters up to 3.6 m and a 15-m submillimetre radio telescope (SEST) are now in operation. The 3.5-m New Technology Telescope (NTT) became operational in 1990, and a giant telescope (VLT = Very Large Telescope), consisting of four 8-m telescopes (equivalent aperture ...
... fourteen optical telescopes with diameters up to 3.6 m and a 15-m submillimetre radio telescope (SEST) are now in operation. The 3.5-m New Technology Telescope (NTT) became operational in 1990, and a giant telescope (VLT = Very Large Telescope), consisting of four 8-m telescopes (equivalent aperture ...
The Mason-Dixon Astronomer - Westminster Astronomical Society, Inc.
... I had just about given up on owning a nice barbell tektite. The ones I have seen on the Internet or at mineral shows just weren’t that good. However, at the Winter Star Party in Florida, there was a dealer that had some meteorites and tektites for sale. I looked over the “barbell” tektites and sever ...
... I had just about given up on owning a nice barbell tektite. The ones I have seen on the Internet or at mineral shows just weren’t that good. However, at the Winter Star Party in Florida, there was a dealer that had some meteorites and tektites for sale. I looked over the “barbell” tektites and sever ...
Astro-figer
... of the massive post-Red Supergiants IRC A ghostly ring stretches seven light-years +10420 and HD 179821, MNRAS 385, around the corpse of a massive star called ...
... of the massive post-Red Supergiants IRC A ghostly ring stretches seven light-years +10420 and HD 179821, MNRAS 385, around the corpse of a massive star called ...
Presentation - National e
... software removed (and with any errors corrected) The logic behind the UOC addresses a Standards defined for future data sets (e.g. STEREO, ILWS, Solar-B) ...
... software removed (and with any errors corrected) The logic behind the UOC addresses a Standards defined for future data sets (e.g. STEREO, ILWS, Solar-B) ...
The Heliophysics Integrated Observatory
... directory structure would make them simpler to access Simple catalogue (textual?) might provide additional information Discussed at VOiG in 2007; IAU WG discussion ...
... directory structure would make them simpler to access Simple catalogue (textual?) might provide additional information Discussed at VOiG in 2007; IAU WG discussion ...
Indian Institute of Astrophysics
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The Indian Institute of Astrophysics (IIA), with its headquarters in Bangalore (Karnataka state), India, is a premier national institute of India for the study of and research into topics pertaining to astronomy, astrophysics and related subjects.The Institute has a network of laboratories and observatories located in various places in India, including Kodaikanal (the Kodaikanal Solar Observatory), Kavalur (the Vainu Bappu Observatory), Gauribidanur, Hanle (the Indian Astronomical Observatory) and Hosakote.