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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.…
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Keywords:
galaxy;
dual agn;
possible sub;
double peaked ... See more keywords
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1
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…
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Keywords:
peaked narrow;
double peaked;
origin double;
agn outflows ... See more keywords
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1
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…
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Keywords:
dual agn;
agn;
double peaked;
binary agn ... See more keywords
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1
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…
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Keywords:
search method;
method based;
profiles search;
double peaked ... See more keywords
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0
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…
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Keywords:
bosscha observatory;
emission stars;
double peaked;
line ... See more keywords