| http://www.w3.org/ns/prov#value | - Express 19, 15690???15695 (2011). [CrossRef] [PubMed] ], there are compelling reasons to observe in the near IR. Because of their relatively low temperature, M dwarf stars, especially M4 and later, are faint in the visible but bright in the near IR (900 nm ??? 1800 nm.) These stars are very good candidates for a radial velocity survey; M dwarf stars make up more than 60% of the stars within 10 pc
|
