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Category | I |
---|---|
Domain name | iistars.com.au |
IP | 223.130.25.180 |
Country by IP | AU |
Web server type | IIS |
Hostname | c2s4-2e-mel.hosting-services.net.au |
iistars is a respected and innovative event management company We are creative, passionate and... 350 Collins Street, South Melbourne, VIC, Australia 3000 Visit website
iistars is a respected and innovative event management company We are creative, passionate and... 350 Collins Street, Australia VIC South Melbourne 3000 Visit website
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The Daily Rewind by Mrs. Smith. Welcome to our class! Why Do I Need to Look at this Website? We are attempting to create a paper free classroom as we are in the digital age. Each week, students are given website assignments that COUNT as a class grade. Students will submit their work electronically and it will automatically come to my computer. Visit website
Statewide Traffic Analysis and Reporting System (STARS II) is a data analysis and reporting database with detailed traffic data and statistics. Visit website
MNRAS000,1–12(2019) Preprint28June2021 CompiledusingMNRASLATEXstylefilev3.0 Highly r-process enhanced stars in ultra-faint dwarf galaxies MyoungwonJeon1 ... Visit website
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(abridged) The star formation rate (SFR) linearly correlates with the amount of dense gas mass (Mdg) involved in the formation of stars both for distant galaxies and clouds in our Galaxy. Similarly, the mass accretion rate (Macc) and the disk mass (Mdisk) of young, Class II stars are also linearly correlated. We plotted the corresponding observational data together, finding a … Visit website
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massasPop IIstars(Bromm etal.2001).Itisthereforenaturalto think thatthesestars may play an importantrolein early reionization.Ironically,lessisknown aboutthe second generation ofstars,precisely becausethemetals,magnetic elds,and photonsproduced by the rststarscomplicate the situation. The key processesthatdetermine how e ciently Visit website
A new r-process star with low abundances of r-process elements A Frebel, Q Yu, H R Jacobson DepartmentofPhysics,MassachusettsInstituteofTechnology&KavliInstitutefor Visit website
2018JINA-CEEFrontiersinNuclearAstrophysics ContributionID:60 Type:poster TheR-ProcessAllianceR-IIStarSurvey Wednesday,May23,20184:30PM(1h30m ... Visit website
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Cloud$Collapse$ • Thermally:supported$non:rotang$cloud$ • Inside:outcollapse$ – R=c s t( c s:sound$speed)$ – m acc =m dot $t – 2Gm acc Visit website
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