Predicted gamma-ray line emission from the Cygnus complex

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Volume 511 (February 2010)

A&A, 511 (2010) A86

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Table 1:

Characteristics of the Cygnus OB associations and stellar clusters collectively referred to as the Cygnus complex (from Knödlseder et al. 2002).
Name	Observed population	Distance (pc)	Age (Myr)
Cyg OB1	23 $\in$ [15, 40 $M_{\odot}$ ]	1905	4
Cyg OB2	120 $\in$ [20, 120 $M_{\odot}$ ]	1584	2.5
Cyg OB3	14 $\in$ [25, 60 $M_{\odot}$ ]	2187	3.5
Cyg OB7	10 $\in$ [7, 25 $M_{\odot}$ ]	832	3.5
Cyg OB8	6 $\in$ [20, 40 $M_{\odot}$ ]	2399	7.5
Cyg OB9	8 $\in$ [20, 40 $M_{\odot}$ ]	1259	3.5
Ber 86	11 $\in$ [7, 25 $M_{\odot}$ ]	1660	4
Ber 87	24 $\in$ [7, 25 $M_{\odot}$ ]	1905	4.5
NGC 6871	13 $\in$ [7, 25 $M_{\odot}$ ]	2399	5.5
NGC 6913	13 $\in$ [7, 40 $M_{\odot}$ ]	1820	3.5
NGC 6910	7 $\in$ [7, 25 $M_{\odot}$ ]	1820	4.5
NGC 6883	2 $\in$ [12, 15 $M_{\odot}$ ]	1820	15
IC 4996	6 $\in$ [6, 25 $M_{\odot}$ ]	1660	5.5

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