New candidate planetary nebulae in M 81

被引:20
作者
Magrini, L
Perinotto, M
Corradi, RLM
Mampaso, A
机构
[1] Univ Florence, Dipartimento Astron & Sci Spazio, I-50125 Florence, Italy
[2] Isaac Newton Grp Telescopes, Santa Cruz De La Palma 38700, Canarias, Spain
[3] Inst Astrofis Canarias, Tenerife 38200, Canarias, Spain
来源
ASTRONOMY & ASTROPHYSICS | 2001年 / 379卷 / 01期
关键词
planetary nebulae; galaxies : M 81; galaxies : ISM;
D O I
10.1051/0004-6361:20011301
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A 34' x 34' field centred on the spiral galaxy M 81 has been searched for emission-line objects using the prime focus wide field camera (WFC) of the 2.54 m Isaac Newton Telescope (La Palma, Spain). A total of 171 candidate planetary nebulae (PNe) are found, 54 of which are in common with the ones detected by Jacoby et al. (1989). The behaviour of PNe excitation as a function of galactocentric distance is examined, and no significant variations are found. The PNe luminosity function is built for the disk and bulge of M 81, separately. A distance modulus of 27.92 +/- 0.23 mag is found for disk PNe, in good agreement with previous distance measurements for M 81. (Jacoby et al. 1989; Huterer et al. 1995).
引用
收藏
页码:90 / 95
页数:6
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