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相关论文: Planetary nebulae and how to find them: A concise …

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Premise: This report is intended to provide useful background and information on how we find detect and compile Planetary Nebulae PNe candidates and then verify them. It is for postgraduate students entering the field and for more general…

星系天体物理 · 物理学 2022-07-06 Quentin A Parker

By incorporating our major recent discoveries with re-measured and verified contents of existing catalogues we provide, for the first time, an accessible, reliable, on-line SQL database for essential, up-to date information for all known…

太阳与恒星天体物理 · 物理学 2016-08-24 Quentin A Parker , Ivan Bojicic , David J Frew

Recent Halpha surveys such as SHS and IPHAS have improved the completeness of the Galactic planetary nebula (PN) census. We now know of ~3,000 PNe in the Galaxy, but this is far short of most estimates, typically ~25,000 or more for the…

Context. There are more than 3000 true and probable known Galactic Planetary Nebulae (PNe), but only for 13% of them there is central star spectroscopic information available. Aims. To contribute to the knowledge of central stars of…

星系天体物理 · 物理学 2015-05-20 Weidmann Walter A. , Roberto Gamen

The Hong Kong/AAO/Strasbourg Halpha (HASH) planetary nebula database is an online research platform providing free and easy access to the largest and most comprehensive catalogue of known Galactic planetary nebulae (PNe) and a repository of…

天体物理仪器与方法 · 物理学 2017-11-15 I. S. Bojicic , Q. A. Parker , D. J. Frew

A detailed examination of new high quality radio catalogues (e.g. Cornish) in combination with available mid-infrared (MIR) satellite imagery (e.g. Glimpse) has allowed us to find 70 new planetary nebula (PN) candidates based on existing…

星系天体物理 · 物理学 2017-11-15 Vasiliki Fragkou , Ivan Bojičić , David Frew , Quentin Parker

We address the general problem of the luminosity-specific planetary nebula (PN) number, defined as alpha = N(PN)/L(gal), and its relationship with age and metallicity of the parent stellar population. Our analysis relies on population…

天体物理学 · 物理学 2009-11-11 A. Buzzoni , M. Arnaboldi , R. L. M. Corradi

Planetary nebulae (PNe) are essential tracers of the kinematics of the diffuse halo and intracluster light where stellar spectroscopy is unfeasible, due to their strong emission lines. However, that is not all they can reveal about the…

星系天体物理 · 物理学 2023-11-16 Ana Ennis , Johanna Hartke , Magda Arnaboldi , Claudia Pulsoni , Fuyan Bian , Chiara Spiniello

Planetary nebulae (PNe) are valuable spatial and kinematic tracers of nearby galaxies. In this mini-review, I focus on their role in tracing the halo and intra-cluster/intra-group light assembly in groups and clusters of galaxies within…

星系天体物理 · 物理学 2025-10-29 Johanna Hartke

We present the first results of our search for new, extended Planetary Nebulae (PNe) based on careful, systematic, visual scrutiny of the imaging data from the INT Photometric H-alpha Survey of the Northern Galactic Plane (IPHAS). The newly…

We have, for the first time, compiled a nearly complete census of planetary nebulae (PNe) centred on the Sun. Our goal is the generation of an unbiased volume-limited sample, in order to answer some long-standing statistical questions…

太阳与恒星天体物理 · 物理学 2010-10-26 David J. Frew , Quentin A. Parker

Planetary nebulae (PNe) provide tests of stellar evolution, can serve as tracers of chemical evolution in the Milky Way and other galaxies, and are also used as a calibrator of the cosmological distance ladder. Current and upcoming large…

太阳与恒星天体物理 · 物理学 2019-07-10 George Vejar , Rodolfo Montez , Margaret Morris , Keivan G. Stassun

We present a supplement to the Macquarie/AAO/Strasbourg H$\alpha$ planetary nebulae (PNe) catalogue (MASH), which we denote MASH-II. The supplement consists of over 300 true, likely and possible new Galactic PNe found after re-examination…

天体物理学 · 物理学 2009-11-13 B. Miszalski , Q. A. Parker , A. Acker , J. L. Birkby , D. J. Frew , A. Kovacevic

Planetary nebulae (PNe) consist of an ionized envelope surrounding a hot central star (CSPN) that emits mostly at ultraviolet (UV) wavelengths. Ultraviolet observations, therefore, provide important information on both the CSPN and the…

太阳与恒星天体物理 · 物理学 2023-06-13 M. A. Gómez-Muñoz , L. Bianchi , A. Manchado

Planetary Nebulae (PNe) have been used satisfactory to test the effects of stellar evolution on the Galactic chemical environment. Moreover, a link exists between nebular morphology and stellar populations and evolution. We present the…

天体物理学 · 物理学 2016-01-27 Letizia Stanghellini

This paper describes how commercially available spectrographs can be used to identify and measure some basic characteristics of planetary nebulae.

太阳与恒星天体物理 · 物理学 2018-07-18 Paul Luckas

We investigate the efficacy of a systematic planetary nebula (PN) search in the Census of the Local Universe (CLU) narrowband (H$\alpha$) survey that covers a considerably larger sky region of above declination $-20^\circ$ than most…

In this review we cover the detection, identification and astrophysical importance of planetary nebulae (PN). The legacy of the historic Perek & Kohoutek and Acker et al. catalogues is briefly covered before highlighting the more recent but…

星系天体物理 · 物理学 2010-11-04 Quentin A. Parker , David J. Frew

Context. We have carried out a semi-automated search for planetary nebulae (PNe) in the INT Photometric H-Alpha Survey (IPHAS) catalogue. We present the PN search and the list of selected candidates. We cross correlate the selected…

Planetary nebulae (PNe) have the potential to revolutionize our understanding of extragalactic stellar populations. Indeed, in many systems, bright PNe are the only individual objects identifiable from the ground, and, even more often, they…

天体物理学 · 物理学 2009-11-11 Robin Ciardullo
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