The past, present and future of Galactic planetary nebula surveys

被引:8
作者
Parker, Quentin A. [1 ,2 ,3 ]
Frew, David J. [1 ,2 ]
Acker, Agnes [4 ]
Miszalski, Brent [5 ]
机构
[1] Macquarie Univ, Dept Phys & Astron, Sydney, NSW 2109, Australia
[2] Macquarie Univ, Res Ctr Astron Astrophys & Astrophoton, Sydney, NSW, Australia
[3] Australian Astron Observ, Epping, NSW 1710, Australia
[4] Observ Astron, F-67000 Strasbourg, France
[5] South African Astron Observ, ZA-7935 Observatory, South Africa
来源
PLANETARY NEBULAE: AN EYE TO THE FUTURE | 2012年 / 283期
关键词
Planetary nebulae: general; catalogs; surveys; infrared: stars; radio continuum: stars; ISM: general; Galaxy: evolution; H-ALPHA SURVEY; SPITZER-SPACE-TELESCOPE; POST-AGB STARS; MAGELLANIC-CLOUD; BULGE REGION; IPHAS; CATALOG; GLIMPSE; DISCOVERIES; WAVELENGTHS;
D O I
10.1017/S1743921312010617
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Over the last decade Galactic planetary nebula discoveries have entered a golden age due to the emergence of high sensitivity, high resolution narrow-band surveys of the Galactic plane. These have been coupled with access to complimentary, deep, multi-wavelength surveys across near-IR, mid-IR. and radio regimes in particular from both ground-based and space-based telescopes. These have provided powerful diagnostic and discovery capabilities. In this review these advances are put in the context of what has gone before, what we are uncovering now and through the window of opportunity that awaits in the future. The astrophysical potential of this brief but key phase of late stage stellar evolution is finally being realised.
引用
收藏
页码:9 / +
页数:3
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