Abstract
We demonstrate here the possibility of using very low dispersion (10000 A mm−1) slitless spectroscopy of stars for a fairly accurate spectral classification. The technique is shown to be very useful in studies of star clusters.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
