Absolute spectrophotometry of northern compact planetary nebulae

被引:19
|
作者
Wright, SA
Corradi, RLM
Perinotto, M
机构
[1] Isaac Newton Grp Telescopes, Santa Cruz de La Palma 38700, Canary Isl, Spain
[2] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[3] Univ Florence, Dipartimento Astron & Sci Spazio, I-50125 Florence, Italy
来源
ASTRONOMY & ASTROPHYSICS | 2005年 / 436卷 / 03期
关键词
ISM : planetary nebulae :; general; techniques : spectroscopic; line : identification; ISM : abundances;
D O I
10.1051/0004-6361:20052666
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present medium-dispersion spectra and narrowband images of six northern compact planetary nebulae (PNe): BoBn 1, DdDm 1, IC 5117, M 1-5, M 1-71, and NGC 6833. From broad-slit spectra, total absolute fluxes and equivalent widths were measured for all observable emission lines. High signal-to-noise emission line fluxes of H alpha, H beta, [OIII], [NII], and HeI may serve as emission line flux standards for northern hemisphere observers. From narrow-slit spectra, we derive systemic radial velocities. For four PNe, available emission line fluxes were measured with sufficient signal-to-noise to probe the physical properties of their electron densities, temperatures, and chemical abundances. BoBn 1 and DdDm 1, both type IV PNe, have an H beta flux over three sigma away from previous measurements. We report the first abundance measurements of M 1-71. NGC 6833 measured radial velocity and galactic coordinates suggest that it is associated with the outer arm or possibly the galactic halo, and its low abundance ([O/H] = 1.3 x 10(-4)) may be indicative of low metallicity within that region.
引用
收藏
页码:967 / 975
页数:9
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