Open clusters - II. Fundamental parameters of B stars in Collinder 223, Hogg 16, NGC 2645, NGC 3114, and NGC 6025

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Volume 577 (May 2015)

A&A, 577 (2015) A45

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Table 7

Hogg 16: Stellar fundamental parameters from the BCD system.

ID	Other	D	λ₁	Φ_b	S.T	T_eff	log g	M_v	M_bol
Vázquez	designation	[dex]	[Å]	[μ]		[K]	[dex]	[mag]	[mag]	[μ]

01	CD−60 4699	0.14	71	1.45	B2VI:	25 455 ± 1586:	4.24 ± 0.06:	−2.25 ± 0.25:	−4.33 ± 0.35:	0.70 ± 0.01
02	CD−60 4696	0.12	39	1.57	B2II	21 618 ± 2177	2.80 ± 0.17:	−4.51 ± 0.84	−5.76 ± 0.67	0.70 ± 0.01
03	CD−60 4701 ^dd	0.10	46	1.54	B1III^Be	24 698 ± 2826	2.98 ± 0.34	−4.38 ± 0.78	−6.13 ± 0.50	0.69 ± 0.01
05	CPD−60 4698	0.43	73	1.58	A0VI:	10 538 ± 334:	4.52 ± 0.11:	−0.06 ± 0.41:	0.11 ± 0.19:	0.99 ± 0.04
06	CPD−60 4695	0.18	49	1.52	B3IV	20 595 ± 1171	3.80 ± 0.31	−2.33 ± 0.51	−3.94 ± 0.47	0.72 ± 0.01
09	CPD−60 4703	0.07	39	2.19	B0Ib^Em	26 817 ± 3586	2.69 ± 0.11:	−6.11 ± 0.91:	−7.61 ± 0.71	0.69 ± 0.01
14	CPD−60 4699	0.35	52	1.20	B8V	12 041 ± 274	4.06 ± 0.18	−0.04 ± 0.26	−0.83 ± 0.26	0.85 ± 0.02
49	HD 117 239	0.51	87	1.30	A2V^mk	9000 ± 500^a	4.20 ± 0.30^a	1.30 ± 0.50^a	1.10 ± 0.50^a	1.12 ± 0.02
50	HD 117 256	0.33	53	1.22	B6V	13 584 ± 505	4.03 ± 0.20	−0.33 ± 0.26	−1.14 ± 0.26	0.80 ± 0.02
52	HD 116 999	0.32	49	1.30	B6IV	13 871 ± 378	3.87 ± 0.25	−0.62 ± 0.36	−1.43 ± 0.38	0.79 ± 0.01
53	CPD−60 4719	0.15	49	1.50	B2III	22 610 ± 1651	3.54 ± 0.36	−2.86 ± 0.54	−4.58 ± 0.44	0.71 ± 0.01
68	HD 116 875 ^dd	0.23	52	1.08	B4V^Be	18 000 ± 826	3.95 ± 0.24	−1.43 ± 0.39	−2.79 ± 0.40	0.75 ± 0.01
74	CPD−60 4711	0.49	73	1.58	A5V:	8180 ± 500^a	4.29 ± 0.30^a	1.95 ± 0.50^a	1.80 ± 0.50^a	1.27 ± 0.06
75	CPD−60 4705	0.42	88	1.66	A5V:	8180 ± 500^a	4.29 ± 0.30^a	1.95 ± 0.50^a	1.80 ± 0.50^a	1.27 ± 0.06

Notes. Nomenclature according to Vazquez & Feinstein (1991). The symbol : is used to indicate extrapolated values. g is the stellar surface gravity given in cm s^-2.

^(dd)

Stars with double Balmer discontinuity.

^(mk)

Spectral types derived using the MK-system.

^(Be)

Known Be star.

^(Em)

Emission line star.

^(a)

Values interpolated from Cox (2000).

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