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

Home

All issues

Volume 577 (May 2015)

A&A, 577 (2015) A45

Full HTML

Free Access

Table 13

NGC 6025: Stellar fundamental parameters from the BCD system.

ID	Other	D	λ ₁	Φ_b	S.T	T _eff	log g	M _v	M _bol
Feinstein	designation	[dex]	[Å]	[μ]		[K]	[dex]	[mag]	[mag]	[μ]
Kilambi

01	HD 143 448	0.06	81	1.20	B0V:^Be	30 000 ± 4275^a	3.94 ± 0.00^a	−4.00 ± 0.64^a	−7.16 ± 0.64^a	0.68 ± 0.01
02	HD 143 449	0.26	47	1.29	B5IV	16 275 ± 531	3.78 ± 0.29	−1.49 ± 0.47	−2.58 ± 0.45	0.76 ± 0.01
03	HD 143 413 ^dd	0.24	43	1.21	B5III	16 780 ± 804	3.46 ± 0.32	−1.87 ± 0.55	−3.07 ± 0.53	0.76 ± 0.01
04	CD−60 6021	0.34	57	1.20	B7V	12 857 ± 491	4.15 ± 0.11	−0.13 ± 0.21	−0.92 ± 0.23	0.82 ± 0.02
05	CD−60 6007	0.36	61	1.17	B7V	12 216 ± 376	4.23 ± 0.13	0.13 ± 0.32	−0.73 ± 0.16	0.85 ± 0.02
06	HD 143 288	0.29	57	1.42	B6V^e	14 750 ± 650	4.19 ± 0.14	−0.45 ± 0.30	−1.59 ± 0.30	0.78 ± 0.01
07	HD 143 340	0.24	44	1.36	B5III	16 607 ± 750	3.49 ± 0.32	−1.81 ± 0.55	−2.92 ± 0.53	0.76 ± 0.01
08	CD−60 6015	0.27	53	1.17	B5V	15 705 ± 628	4.04 ± 0.19	−0.84 ± 0.32	−2.08 ± 0.33	0.77 ± 0.01
11	HD 143 287	0.31	55	1.23	B6V^p	13 805 ± 522	4.11 ± 0.17	−0.35 ± 0.20	−1.33 ± 0.28	0.80 ± 0.01
12	HD 143 309	0.20	48	1.23	B3IV^v	19 386 ± 1081	3.70 ± 0.32	−2.19 ± 0.51	−3.55 ± 0.45	0.73 ± 0.01
13	CD−60 6011	0.28	49	0.97	B5IV	15 558 ± 594	3.85 ± 0.26	−0.93 ± 0.41	−2.04 ± 0.42	0.77 ± 0.01
14	CD−60 6013	0.27	55	1.07	B6V	15 575 ± 554	4.10 ± 0.17	−0.74 ± 0.28	−1.87 ± 0.30	0.77 ± 0.01
15	CD−60 6017	0.31	77	2.23	F0V:	7300 ± 700^a	4.34 ± 0.50^a	2.70 ± 0.50^a	2.61 ± 0.50^a	1.67 ± 0.03
16	CD−60 6027	0.31	51	1.38	B6V	14 017 ± 453	3.97 ± 0.22	−0.57 ± 0.34	−1.54 ± 0.35	0.79 ± 0.01
22	HD 143 388	0.24	50	1.18	B4IV	17 379 ± 692	3.87 ± 0.26	−1.46 ± 0.41	−2.74 ± 0.44	0.75 ± 0.01
23	CD−60 6024	0.25	48	1.29	B4IV	16 696 ± 659	3.81 ± 0.28	−1.45 ± 0.43	−2.58 ± 0.50	0.76 ± 0.01
24	CPD−59 6562	0.34	60	1.39	B7V	13 090 ± 490	4.23 ± 0.13	0.03 ± 0.31	−0.89 ± 0.19	0.83 ± 0.02
25	HD 143 412 ^dd	0.31	59	1.39	B7V^p	14 316 ± 714	4.22 ± 0.13	−0.26 ± 0.25	−1.21 ± 0.20	0.80 ± 0.01
26	V 396 Nor	0.46	70	1.55	A1V^EB	9938 ± 376	4.39 ± 0.10:	0.52 ± 0.22:	0.27 ± 0.32^a	1.02 ± 0.04
43	HD 143 123	0.25	53	1.40	B4V	17 010 ± 770	4.02 ± 0.21	−1.08 ± 0.36	−2.39 ± 0.33	0.76 ± 0.01
86	CPD−60 6287	0.48	79	1.60	A2:VI:	9540 ± 318:	4.20 ± 0.30^a	1.30 ± 0.50^a	1.10 ± 0.50^a	1.12 ± 0.05
90	HD 143 027	0.27	45	1.46	B5IV^p	15 705 ± 583	3.66 ± 0.29	−1.41 ± 0.48	−2.37 ± 0.52	0.77 ± 0.01

Notes. Nomenclature according to Feinstein (1971) and Kilambi (1975). 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.

^(Be)

Known Be stars.

^(e)

Hβ in emission, reported by Grosso & Levato (2011).

^(p)

Reported as peculiar star.

^(EB)

Eclipsing binary star.

^(v)

Variable star.

^(a)

Values interpolated from Cox (2000).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.