Stars and dust in the Galactic Center
... Binned velocity dispersion used for Jeans modeling . . . . . . . Radial and tangential dispersions as function of the radius . . . Average radial velocities from our data and the literature . . . . Data and fits of the Jeans modeling . . . . . . . . . . . . . . . . Binwise median and maximum three-di ...
... Binned velocity dispersion used for Jeans modeling . . . . . . . Radial and tangential dispersions as function of the radius . . . Average radial velocities from our data and the literature . . . . Data and fits of the Jeans modeling . . . . . . . . . . . . . . . . Binwise median and maximum three-di ...
arXiv:astro-ph/0702414v1 15 Feb 2007
... The observations were obtained with FORS2 at the VLT UT4 using the holographic grisms 1400V and 1200R. The spectral resolution was R ≈ 2000. The spectral range of the 1400V (1200R) grism was about 4500 to 5800 (5700 to 7300) Å. The central wavelengths depend on the target position in the focal plane ...
... The observations were obtained with FORS2 at the VLT UT4 using the holographic grisms 1400V and 1200R. The spectral resolution was R ≈ 2000. The spectral range of the 1400V (1200R) grism was about 4500 to 5800 (5700 to 7300) Å. The central wavelengths depend on the target position in the focal plane ...
this article
... images were obtained using the narrowband line-free filter centered at 6487 8 (k ¼ 67 8). Three exposures of 1200 s were obtained through each of the line and continuum filters. Details of the observations are summarized in Table 2. Three galaxies were imaged using the Seaver Prototype Imaging came ...
... images were obtained using the narrowband line-free filter centered at 6487 8 (k ¼ 67 8). Three exposures of 1200 s were obtained through each of the line and continuum filters. Details of the observations are summarized in Table 2. Three galaxies were imaged using the Seaver Prototype Imaging came ...
Th`ese d`astrophysique Chemodynamical Simulations of Evolution
... For a long time galaxies were thought to be “spiral nebulae”, because of their unresolved nature with the available technology of the epoch. In the late 1910’s a few clues arose to show the distant nature of these objects. They scientifically credited the idea first proposed by Kant of “island unive ...
... For a long time galaxies were thought to be “spiral nebulae”, because of their unresolved nature with the available technology of the epoch. In the late 1910’s a few clues arose to show the distant nature of these objects. They scientifically credited the idea first proposed by Kant of “island unive ...
Cosmic Rays
... Direct Measurement of CR Age Secondary Isotopes with lifetime ~esc can be used to directly measure the age of CR ...
... Direct Measurement of CR Age Secondary Isotopes with lifetime ~esc can be used to directly measure the age of CR ...
Observational motivation for Dark Matter
... Dark Matter in clusters Dark Matter in Galaxies Cosmological Dark Matter Alternatives ...
... Dark Matter in clusters Dark Matter in Galaxies Cosmological Dark Matter Alternatives ...
DCC - LIGO Document Control Center Portal
... Adapted from “The Blue Marble: Land Surface, Ocean Color and Sea Ice” at visibleearth.nasa.gov NASA Goddard Space Flight Center Image by Reto Stöckli (land surface, shallow water, clouds). Enhancements by Robert Simmon (ocean color, compositing, 3D globes, animation). Data and technical support: MOD ...
... Adapted from “The Blue Marble: Land Surface, Ocean Color and Sea Ice” at visibleearth.nasa.gov NASA Goddard Space Flight Center Image by Reto Stöckli (land surface, shallow water, clouds). Enhancements by Robert Simmon (ocean color, compositing, 3D globes, animation). Data and technical support: MOD ...
U P C NIVERSITAT
... Overall, the challenging, unsolved stellar progenitor problem for SNe Ia stands in marked contrast to the case of core-collapse supernovae, whose stellar progenitors are highly-luminous, massive stars. Observational evidence favors the double-degenerate channel, but significant discrepancies exist b ...
... Overall, the challenging, unsolved stellar progenitor problem for SNe Ia stands in marked contrast to the case of core-collapse supernovae, whose stellar progenitors are highly-luminous, massive stars. Observational evidence favors the double-degenerate channel, but significant discrepancies exist b ...
Local Universe Supernovae and Their Host Galaxies
... Catania Observatory (Italy): M. Turatto CNR-IRA (Italy): F. Mannucci IAP (Paris, France): D. Kunth, G. Mamon INAF-OAC (Italy): M. Della Valle Padova Observatory (Italy): E. Cappellaro, H. Navasardyan, STScI: R. Allen, C. Leitherer, J. MacKenty, B. McLean, N. Panagia ...
... Catania Observatory (Italy): M. Turatto CNR-IRA (Italy): F. Mannucci IAP (Paris, France): D. Kunth, G. Mamon INAF-OAC (Italy): M. Della Valle Padova Observatory (Italy): E. Cappellaro, H. Navasardyan, STScI: R. Allen, C. Leitherer, J. MacKenty, B. McLean, N. Panagia ...
Cepheids
... features will be found compared to the responsible for crossing theory) • Perspective tool to identify crossing number and to refine the P-L relation… ...
... features will be found compared to the responsible for crossing theory) • Perspective tool to identify crossing number and to refine the P-L relation… ...
