"The Pulsar Menagerie" (pdf file)
... dead star known to have a planetary system. The pulsar is special in another way, too: Further analysis of its signals revealed a closely orbiting third planet, much smaller than the other two. The masses and relative positions of the three planets are “shockingly similar to our inner solar system,” ...
... dead star known to have a planetary system. The pulsar is special in another way, too: Further analysis of its signals revealed a closely orbiting third planet, much smaller than the other two. The masses and relative positions of the three planets are “shockingly similar to our inner solar system,” ...
Building a Better Flat-Field: An Instrumental Telescope
... Amali L. Vaz Submitted to the Department of Physics on January 14, 2011, in partial fulfillment of the requirements for the degree of Bachelor of Science in Physics ...
... Amali L. Vaz Submitted to the Department of Physics on January 14, 2011, in partial fulfillment of the requirements for the degree of Bachelor of Science in Physics ...
transparencies - Rencontres du Vietnam
... 2 different Monte-Carlo have been computed to estimate our detection efficiency: _ simulated microlensing effect on true light curve _ fake images that pass all the photometric chain with simulated microlensed star ► they are in excellent agreement for the bright star sample. ...
... 2 different Monte-Carlo have been computed to estimate our detection efficiency: _ simulated microlensing effect on true light curve _ fake images that pass all the photometric chain with simulated microlensed star ► they are in excellent agreement for the bright star sample. ...
Rich Clusters of Galaxies
... evolution. We can compare galaxy evolution in rich clusters with that in lowdensity environments. They provide constraints on the distribution and the amount of dark matter which is needed to bind the clusters. They also are important as gravitational telescopes because of their lensing effect on mu ...
... evolution. We can compare galaxy evolution in rich clusters with that in lowdensity environments. They provide constraints on the distribution and the amount of dark matter which is needed to bind the clusters. They also are important as gravitational telescopes because of their lensing effect on mu ...
Galactic Evolution - Harvard-Smithsonian Center for Astrophysics
... underway today as a kind of evolutionary process (see next section below) that continues well after the foremost galaxy-building events began. Reality may also be somewhere in between these two grand ideas— such as the prospect, now favored in the astronomical community, that the inner core and bulg ...
... underway today as a kind of evolutionary process (see next section below) that continues well after the foremost galaxy-building events began. Reality may also be somewhere in between these two grand ideas— such as the prospect, now favored in the astronomical community, that the inner core and bulg ...
... – Stars travel around the center of the galaxy in their own orbits – Stars and gas traveling in the disc will bunch up as they enter an arm and will spread out as they leave – This bunching is similar to that of cars on a freeway except gravity causes the bunching of the stars – Gas entering the arm ...
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, ...
Massive z~1.3 evolved galaxies revealed
... shown in Fig. 1 (upper panel and lower panel respectively) along with the relevant mean sky residuals. Filled symbols are the photometric data in the I, J and K bands (see Table 1) from the MUNICS survey (Drory et al. 2001). The spectra are normalized to the K-band flux. As an independent check on ...
... shown in Fig. 1 (upper panel and lower panel respectively) along with the relevant mean sky residuals. Filled symbols are the photometric data in the I, J and K bands (see Table 1) from the MUNICS survey (Drory et al. 2001). The spectra are normalized to the K-band flux. As an independent check on ...
