Determination of the stellar parameters of C-rich hydrostatic stars from spectro-interferometric observations

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Table 1

Target list, available photometry, and variability information.

ID	RA	Dec	J	H	K	L	f_{[12 μm]}	Var. type	Amplitude	Period
			[mag]	[mag]	[mag]	[mag]	[Jy]		[mag]	[days]

CR Gem	06:34:23.92	+16:04:30.30	3.36	2.07	1.46	0.88^a	39.31	Lb	1.20 B	250
HK Lyr	18:42:50.00	+36:57:30.89	3.23	2.15	1.62	0.99^b	22.74	Lb	0.40 V^e	186^e
RV Mon	06:58:21.49	+06:10:01.50	3.06	1.96	1.43	0.85^c	31.13	SRb	2.19 B	131
Z Psc	01:16:05.03	+06:10:01.50	2.11	1.10	0.70	0.41^d	33.42	SRb	1.30 p	144
DR Ser	18 47 21.02	+05 27 18.60	4.12	2.79	2.08	1.38^a	15.9	Lb	0.50 V^f	196^f

Notes. The amplitude and the period (unless otherwise stated) are derived from the General Catalogue of Variable Stars (GCVS; Samus+ 2007 − 2009). The band used for amplitude of variability measurement is also reported; “p” denotes photographic plates.

^(a)

Kerschbaum et al. (1996a);

^(b)

Kerschbaum et al. (1996b);

^(c)

Epchtein et al. (1990);

^(d)

Bagnulo (1996);

^(e)

Beichman et al. (1988);

^(f)

Pojmanski (2002).

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