[vsnet-alert 22145] Re: Gaia18bec

roberto nesci Roberto.Nesci at iaps.inaf.it
Tue May 8 14:48:01 JST 2018


The 2MASS colors (J-H=0.97, H-K=0.48are typical of a very late M giant, an AGB 
star likely variable (Mira, SR).
Roberto Nesci


On 8/05/18 7:01 AM, Taichi Kato wrote:
> 278.42666	-14.23112	

-- 
prof. Roberto Nesci,  associated to Istituto Nazionale di Astrofisica,
(National Institute of Astrophysics) INAF-IAPS, via Fosso del Cavaliere 100, 
00133 Roma, Italia



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