Observation and modelling of main-sequence star chromospheres - IX. Two-component model chromospheres for nine M1 dwarfs

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Volume 509 (January 2010)

A&A, 509 (2010) A65

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Table 4:

Column mass at the transition region and spectral line equivalent widths for quiescent regions and plages for the near-solar metallicity stars of this paper.
Star	f	CaII EW	CaII EW	H $_{\alpha }$ EW	H $_{\alpha }$ EW	log(column mass)	log(column mass)
		Quiescent regions	Active regions	Quiescent regions	Active regions	Quiescent regions	Active regions
	(%)	(Å)	(Å)	(Å)	(Å)	(g cm^-2)	(g cm^-2)
Gl 2	9 $~\pm~$ 2	-0.967	-4.84	0.559	-0.251	-4.450	-4.026
GJ 1010A	32 $~\pm~$ 62	-0.081	-0.405	0.300	0.552	-5.200	-4.604
Gl 49	26 $~\pm~$ 29	-1.17	-5.83	0.551	-0.591	-4.299	-3.886
Gl 150.1B	37 $~\pm~$ 40	-0.564	-2.82	0.573	0.253	-4.500	-4.072
Gl 205	15 $~\pm~$ 22	-0.884	-4.42	0.566	-0.133	-4.375	-3.964
Gl 229	28 $~\pm~$ 42	-0.477	-2.38	0.560	0.349	-4.550	-4.111
Gl 526	36 $~\pm~$ 46	-0.203	-1.02	0.478	0.557	-4.800	-4.337
G192-11A	29 $~\pm~$ 25	-1.12	-5.59	0.553	-0.458	-4.311	-3.903
Gl 880	37 $~\pm~$ 27	-0.477	-2.38	0.560	0.349	-4.550	-4.111

Source LaTeX | All tables | In the text

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