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stellar population results from nfps: age and metallicity along the red sequence russell smith (waterloo), jenica nelan (dartmouth), mike hudson (waterloo), steve moore (durham),…
stellar population results from nfps: age and metallicity along the red sequence russell smith (waterloo), jenica nelan (dartmouth), mike hudson (waterloo), steve moore (durham),…
slide 1stellar population results from nfps: age and metallicity along the red sequence russell smith (waterloo), jenica nelan (dartmouth), mike hudson (waterloo), steve…
stellar-mass metallicity relation at high redshifts stellar-mass metallicity relation at high redshifts stellar-mass metallicity relation at z~1.4 kouji ohta (kyoto…
slide 1stellar-mass metallicity relation at high redshifts stellar-mass metallicity relation at z~1. 4 kouji ohta ( kyoto university ) k. yabe, f. iwamuro, s.…
stellar metallicity of the extended disk and distance of the spiral galaxy ngc 3621 rolf-peter kudritzki12 institute for astronomy university of hawaii 2680 woodlawn drive…
metallicity effect on stellar granulation detected from red giants in open clusterss . m at h u r , r . a . g a r c a , p. g a u l m e , m . p i n s o n n e a u lt, k . s…
lecture on stellarbinary evolution population synthesis ashley ruiter max planck institute for astrophysics garching, germany [email protected] mon. january 18 2010…
stellar population synthesis – basic methodology and examples on star formation rate and metallicity steffen silies email: steffensilies@uni-bielefeldde 20082018 contents…
ar x iv :0 80 4 28 92 v2 as tr o- ph 6 m ay 2 00 8 mon not r astron soc000 1–15 2008 printed 22 october 2018 mn latex style file v22 on the galaxy stellar mass function…
spectrographs part 1 ati 2014 lecture 10 kenworthy and keller the solar spectrum design drivers for spectrographs what spectral resolution do you need? what bandwidth wavelength…
spectral indices broad band colors are affected by the age-metallicity degeneracy spectral indices have been introduced to overcome this problem lectures on stellar populations…
aa ultracompact ns-ns: tmerger ~ 1-100 myr detailed single stellar models wind-, metallicity-dependent evolution binary component tidal interactions ang. momentum loss: gr,…
the new filipino private school sharjah, united arab emirates baccalaureate mass 2015 music for the mass entrance hymns the lord is present in his sanctuary the lord is present…
fred nuclear physics and low-metallicity stellar abundances: victories and struggles chris sneden, university of texas speaking on behalf of many friends and colleagues in…
distances to galaxies from the brightest stars in the universe rolf kudritzki in collaboration with miguel urbaneja fabio bresolin vivian uzach gazak requires independent…
1. the blueprint for crm an approach for nfp organisations 2. what are the key concerns? research has shown that the most significant concerns in introducing crm in are:…
8/8/2019 nfps uniform order form 1/3c:\documents and settings\bec\my documents\rebecca\nfps school council\2010 projects\website\other forms\uniform order form 2010 updated…
institute of astrophysics and space sciences nuno c santos nunosantos@astrouppt characterisation of exoplanet host stars a window into planet formation nuno c santos…
slide 1 metallicity dependent wolf-rayet winds metallicity dependent wolf-rayet winds paul crowther slide 2 introduction wolf-rayet (wr) stars represent the final phase…