GS100-02-41: a new large H i shell in the outer part of the Galaxy

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Table 3

Cep OB1 stars lying inside GS 100–02–41.

Star	l	b	Sp. Type	MS Sp. Type	MS lifetime (Myr)	log (Ṁ (M_⊙ yr^-1))	V_w (km s^-1)	E_w(10⁵⁰ erg)

HDE 235673	984	–16	O6.5 V	O6.5	5.6	–6.27	2700	≤2.2
HD 209678	993	–18	B2 I	B0	12	–7.17	1600	0.2
HD 209900	997	–17	A0 Ib	B1	26	–8.2	2500	0.2
HD 210809	999	–31	O9 Iab	O7	6.4	–6.39	2700	2.1
BD +51 3135	1006	–21	B3 II	B0.5	14	–7.3	1850	0.2
HDE 235781	1012	–26	B6 Ib	B1	22	–8.2	2500	0.2
BD +53 2820	1012	–17	B0 IV	B0	16	–7.17	1600	0.2
BD +52 2833	1014	–21	B1 III	O9.5	10	–7.04	2500	0.5
BD +53 2837	1015	–21	B2 III	B0.5	14	–7.3	1850	0.2
HDE 235783	1017	–19	B1 Ib	B0.5	14	–7.3	1850	0.2
BD +53 2843	1018	–22	O8 III	O7	6.4	–6.39	2700	2.1
BD +54 2718	1020	–09	B2 III	B0.5	14	–7.3	1850	0.2
BD +54 2726	1022	–10	B1.5 II	B0.5	14	–7.3	1850	0.2
HDE 235813	1024	–20	B0 III	O6	6.3	–6.14	2700	2.6
HILTNER 1106	1025	–07	B0 III	O8	6.9	–6.65	2600	0.9
BD +53 2885	1027	–29	B2 III	B0.5	14	–7.3	1850	0.2
HD 212455	1028	–17	B6 Ib	B0.5	14	–7.3	1850	0.2
HDE 235825	1029	–18	O9 V	O9	8	–6.91	2500	≤0.6
BD +54 2764	1030	–17	B1 Ib	B0.5	14	–7.3	1850	0.2
BD +54 2761	1031	–14	O6 III	O3*	4.3	–5.43	3200	≤16.3

References. * The bolometric magnitude and effective temperature given by Garmany & Stencel (1992) lie outside the evolutionary tracks of Schaller et al. (1992). We adopted the earliest spectral type for this star.

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