... Bojan Nikolic web pages (r. 329) . A gallery of interacting galaxies . ... The history of star formation and mass assembly in early-type galaxies . ... Abstract . ... Complete plots of radiospec analysis . Analysis of (radio) spectra . ... Nested Sampling in R & analysis of spectra . ... Paper II: Spinning dust in galaxies . ... The search results are restrict to these pages only . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

... Keywords: globular clusters,M3,photometry,HST . ... Perform the most accurate test of the ``stellar clock'' used in dating globular clusters. ... These data will provide the first complete sample of post-main sequence stars over the entire area of the cluster, and will allow the most stringent tests of stellar evolution and dynamics models. ... M3 contains the largest population of Blue Straggler Stars (BSS) detected in a globular cluster so far ( ). ...

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies using ALMA calibrator observations . ... ALMA . ... ESO-MIDAS . ... It is therefore essential to probe the evolution of cold gas over cosmic time. ... We are looking for an enthusiastic PhD student who is interested in working with us in using ALMACAL to address exciting and topical science questions related to the evolution of molecular gas in galaxies. ...

... Up: Software Systems and Tools . ... The Starlink Software is a collection of astronomical packages and utilities comprising over 120 separate components. When built, the system needs between 500 and 650 MB disk space (without source) making it ideal for distribution on CD-ROM. Each component has been individually packaged into an easy-to-install bundle for users to obtain over the Internet via a ``point and click'' WWW interface from the Starlink Software Store. ...

Next: Other Activities Up: M.E. Bailey Previous: M.E. Bailey Contents . Jonathan Horner, a former summer student at Armagh (now at the University of Bern, Switzerland), Wyn Evans (University of Cambridge) and Mark Bailey have completed two papers on the dynamical evolution of outer solar system objects known as Centaurs. These are large, so-called `giant' comets, circulating on dynamically unstable orbits confined approximately between the orbits of Jupiter and Neptune. ...

... HI gas in the Magellanic Clouds, . ... The Australian Academy of Science are supporting the 'Elizabeth and Frederick White conference on the Magellanic System'. ... The Magellanic Clouds as a template for the study of stellar populations and galaxy interaction . Download: pdf . ... Dating Young Stellar Objects in the Magellanic Clouds . ... The Extended population of the Large Magellanic Cloud . ... Spectral Diagnostics of newly Discovered Planetary Nebulae in the Large Magellanic Cloud . ...

... We show the analysis of low-hard and intermediate states of sources XTE J1550-564, H 1743-322, GX 339-4, XTE J1859-226, XTE J1650-500 and GRS 1915+105. ... Directly applying the scaling technique we also obtain that a ratio of the BH masses in XTE J1859-226 and in XTE J1550-564 is , and the corresponding ratio for XTE J1650-500 and XTE J1550-564 is . These values of scaling factors r implies that BH masses are ; solar masses in XTE J1859-226 and XTE J1650-500 respectively. ...

XMM-Newton Science Analysis System . ... odfingest requires access to a complete ODF. ODF components must comply with the ODF file naming convention. The only ODF component that is required to be present is the ODF summary file. ... All instrument data files found in the ODF directory are analyzed to determine the structure of the observation in terms of active instrument and exposures. If any instrument science file is found, then all the corresponding housekeeping files must be present. ...

Abstract -- The strengths of magnetic fields in interstellar gas clouds are obtained through observations of the circular polarization of spectral line radiation. ... To infer information about these irregularities from the observational data, we develop statistical relationships between the rms values of the irregular component of the magnetic field and spatial variations in the circular polarization of the spectral line radiation. ...

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...