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Questions related from Rajeev Singh Rathour
Object with Teff around 4100 K is not within the computed results of Girardi tracks and isochrones. Any other resource for cool stars?
21 February 2018 8,508 0 View
Any mathematical relation between core mass and envelope mass of Giants (for low or intermediate mass stars)? Also any age-metallicity relation applying to the above case?
21 February 2018 6,179 1 View
The use of line abundance analysis using equivalent width and Kurucz model atmospheres in MOOG code is something done for chemical abundance analysis in stellar astronomy. However there is no...
08 January 2018 5,150 2 View
What are the best possible procedures of correcting for radial velocity in metal poor star having [Fe/H] around -2. We use arcturus spectra as reference but at Teff 4000K and lower metallicity it...
18 December 2017 9,042 0 View