The Distance to NGC 6397 by M-Subdwarf Main-Sequence Fitting
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1538-3881/116/i=6/a=2929/pdf
Reference68 articles.
1. A Spectroscopic Method of Determining the Absolute Magnitudes of A-Type Stars and the Parallaxes of 544 Stars
2. Multicolor NTT CCD photometry of the post-core-collapse globular cluster NGC 6397.
3. Model atmospheres for M (sub)dwarf stars. 1: The base model grid
4. CCD Stromgren studies in NGC 6397
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3. Mean proper motions, space orbits, and velocity dispersion profiles of Galactic globular clusters derived fromGaiaDR2 data;Monthly Notices of the Royal Astronomical Society;2018-11-10
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