NEW Hα STARS. NGC 6910 REGION. II.

被引:1
|
作者
Melikian, N. D. [1 ]
Tamazian, V. S. [2 ]
Karapetian, A. A. [1 ]
Samsonian, A. L. [1 ]
Kostandian, G. R. [1 ]
机构
[1] VA Ambartsumyan Byurakan Astrophys Observ, Byurakan, Armenia
[2] Univ Santiago de Compostela, Ramon Maria Aller Astron Observ, Santiago De Compostela, Spain
关键词
H alpha objects-individual: NGC 6910; EMISSION;
D O I
10.1007/s10511-011-9172-y
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A search for H alpha objects in four fields with an overall area of about 0.14 square degrees in the region of NGC 6910 (the core of the known Cyg OB9 association) has led to the discovery of 64 emission stars, of which 49 are newly detected. The high surface density is indicative of a very rich T association or, possibly, of the projection of several T associations onto one another in this direction. The latter possibility is also indicated by the range of the R photometric stellar magnitudes of the emission stars, 9(m).68-19(m).42. A comparison with earlier observations shows that for many of the stars, the emission line intensity is variable. A P Cyg H alpha line profile is recorded for the star V 1515 Cyg with an emission component equivalent width that greatly exceeds the equivalent absorption width.
引用
收藏
页码:203 / 213
页数:11
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