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Classification parameters for the emission-line spectra of extragalactic objects

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Baldwin, J. A., Phillips, M. M., Terlevich, R.·1981·Publications of the Astronomical Society of the Pacific

Abstract

An investigation is made of the merits of various emission-line intensity ratios for classifying the spectra of extragalactic objects. It is shown empirically that several combinations of easily-measured lines can be used to separate objects into one of four categories according to the principal excitation mechanism: normal H II regions, planetary nebulae, objects photoionized by a power-law continuum, and objects excited by shock-wave heating. A two-dimensional quantitative classification scheme is suggested.

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Metadata

Authors
Baldwin, J. A., Phillips, M. M., & Terlevich, R.
Venue
Publications of the Astronomical Society of the Pacific
Published
1981-02
Volume
93
Pages
5
ISSN
  • 0004-6280 (ISSN-L)
  • 1538-3873
OpenAlex
W1967876247
Cited by
5,132
References
0
FWCI
5.38
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Classification parameters for the emission-line spectra of extragalactic objects. https://app.cochat.ai/papers/10.1086/130766
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Baldwin, J. A., Phillips, M. M., & Terlevich, R. (1981). Classification parameters for the emission-line spectra of extragalactic objects. Publications of the Astronomical Society of the Pacific. https://doi.org/10.1086/130766

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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