Articles with "double peaked" as a keyword



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A possible sub-kiloparsec dual AGN buried behind the galaxy curtain

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Published in 2021 at "Astronomy and Astrophysics"

DOI: 10.1051/0004-6361/202039576

Abstract: Although thousands of galaxy mergers are known, only a handful of sub-kiloparsec-scale supermassive black hole (SMBH) pairs have been confirmed so far, leaving a huge gap between the observed and predicted numbers of such objects.… read more here.

Keywords: galaxy; dual agn; possible sub; double peaked ... See more keywords
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The origin of double-peaked narrow lines in active galactic nuclei - III. Feedback from biconical AGN outflows

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Published in 2018 at "Monthly Notices of the Royal Astronomical Society"

DOI: 10.1093/mnras/stx2433

Abstract: We apply an analytic Markov Chain Monte Carlo model to a sample of 18 AGN-driven biconical outflows that we identified from a sample of active galaxies with double-peaked narrow emission lines at z < 0.1… read more here.

Keywords: peaked narrow; double peaked; origin double; agn outflows ... See more keywords
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Searching for dual AGN in galaxies with double-peaked emission line spectra using radio observations

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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"

DOI: 10.1093/mnras/stz334

Abstract: Supermassive black hole (SMBH) binaries form due to galaxy mergers and minor accretion events. When the SMBHs are accreting, they form dual or binary AGN and can give rise to double-peaked emission lines in the… read more here.

Keywords: dual agn; agn; double peaked; binary agn ... See more keywords
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DoPS: A Double-Peaked Profiles Search Method Based on the RS and SVM

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Published in 2019 at "IEEE Access"

DOI: 10.1109/access.2019.2927251

Abstract: The double-peaked profiles in spectral data are very rare and valuable for the astronomers. Their recognitions are largely depended on visually inspect. The main reasons for auto-search of such spectra are the complex and distinct… read more here.

Keywords: search method; method based; profiles search; double peaked ... See more keywords

B-emission Stars in Southern Sky Observed in Bosscha Observatory: Spectroscopic Study of Hα Spectral Line Variability

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Published in 2019 at "Journal of Mathematical and Fundamental Sciences"

DOI: 10.5614/j.math.fund.sci.2019.51.3.3

Abstract: Hα  line variations of 8 B-emission (Be) stars are presented. Stars that are listed in the Bright Star Catalogue were observed in 2009 at the Bosscha Observatory, Lembang, Indonesia. It was found that 4 stars… read more here.

Keywords: bosscha observatory; emission stars; double peaked; line ... See more keywords