论文标题

Grantecan光谱观测和确认北银河平面中的行星星云候选者

Grantecan spectroscopic observations and confirmations of Planetary Nebulae candidates in the Northern Galactic Plane

论文作者

Ritter, A., Parker, Q. A., Sabin, L., Dû, P. Le, Mulato, L., Patchick, D.

论文摘要

我们提出了10 m望远镜(GTC)的GranteCan光谱镜确认,对我们的Pro-AM协作在Int光度h $_α$调查中很大程度上发现了55个微弱的行星星云(PNE)候选候选者。我们确认其中46个为“ true”(t),4为“可能”(l)和5个为“可能的”(P)PNE,包括5个新的PNE Central Star(CSPN)发现。这是从62名新候选人的观察结果中产生的最大PN发现成功率为89%。 IPHAS的灵敏度和较长的波长覆盖范围可以在更大的灭绝区域,在这些较低的银河纬度区域中发现PNE,包括与先前已知的银河pne相比,在更先进的进化状态和较大的距离处发现了PNE。我们使用一组观察到的特征和光学发射线诊断来确认候选者。血浆特性已经使用pyneb以一种自洽的方式确定。我们强大的多波长数据库“哈希”的功能为这项工作提供了促进(香港,澳大利亚天文天文台,斯特拉斯堡天文台天文台H-alpha行星星云目录),该仪表率是已知的成像,光谱,光谱和其他相关数据,用于所有银色的t,l,p pne和其他相关数据。在可能的情况下,为这些新的PNE提供了红粉,校正的径向速度以及PNE电子密度和温度估计。

We present Grantecan 10 m telescope (GTC) spectroscopic confirmations of 55 faint Planetary Nebulae (PNe) candidates discovered largely in the INT Photometric H$_α$ Survey of the Northern Galactic Plane (IPHAS) by our pro-am collaboration. We confirm 46 of them as 'True' (T), 4 as 'Likely' (L) and 5 as 'Possible' (P) PNe and including 5 new PNe central star (CSPN) discoveries. This was from observations of 62 new candidates yielding a maximum PN discovery success rate of 89%. The sensitivity and longer wavelength coverage of IPHAS allows PNe to be found in regions of greater extinction and at these lower Galactic latitudes, including PNe in a more advanced evolutionary state and at larger distances compared to previously known Galactic PNe. We use an holistic set of observed characteristics and optical emission-line diagnostics to confirm candidates. Plasma properties have been determined in a self-consistent way using PyNeb. This work is facilitated by the functionality of our powerful, multi-wavelength database 'HASH' (Hong Kong, Australian Astronomical Observatory, Strasbourg Observatory H-alpha Planetary Nebula catalogue) that federates known imaging, spectroscopy and other pertinent data for all Galactic T, L, P PNe and the significant numbers of mimics. Reddenings, corrected radial velocities and PNe electron density and temperature estimates are provided for these new PNe where possible.

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