Search Results - "Trippe, M. L"
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A Multi-wavelength Study of the Nature of Type 1.8/1.9 Seyfert Galaxies
Published in The Astrophysical journal (20-12-2010)“…We focus on determining the underlying physical cause of a Seyfert galaxy's appearance as type 1.8 or 1.9. Are these 'intermediate' Seyfert types typical…”
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2
Physical Conditions in the Ultraviolet Absorbers of IRAS F22456–5125
Published in The Astrophysical journal (20-04-2010)Get full text
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Physical Conditions in the Inner Narrow-Line Region of the Seyfert 2 Galaxy Markarian 573
Published in The Astrophysical journal (10-06-2009)“…We have examined the physical conditions within a bright emission-line knot in the inner narrow-line region (NLR) of the Seyfert 2 galaxy Mrk 573 using optical…”
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XMM FOLLOW-UP OBSERVATIONS OF THREE SWIFT BAT-SELECTED ACTIVE GALACTIC NUCLEI
Published in The Astrophysical journal (01-08-2011)“…We present XMM-Newton observations of three active galactic nuclei (AGNs) taken as part of a hunt to find very heavily obscured Compton-thick AGNs. For…”
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5
Joint Hα and X-Ray Observations of Massive X-Ray Binaries. III. The Be X-Ray Binaries HDE 245770 = A0535+26 and X Persei
Published in The Astrophysical journal (10-05-2007)“…We present results from an H alpha monitoring campaign of the Be X-ray binary systems HDE 245770 = A0535+26 and X Per. We use the H alpha equivalent widths…”
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6
Three active galactic nuclei close to the effective Eddington limit for dusty gas
Published in Monthly notices of the Royal Astronomical Society (01-06-2013)“…The effective Eddington limit for dusty gas surrounding active galactic nucleus (AGN) is lower than the canonical Eddington limit for hydrogen gas. Previous…”
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Three AGN Close To The Effective Eddington Limit
Published 28-02-2013“…The Effective Eddington Limit for dusty gas surrounding AGN is lower than the canonical Eddington limit for hydrogen gas. Previous results from the Swift/BAT…”
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XMM Follow-Up Observations of Three Swift BAT-Selected Active Galactic Nuclei
Published 04-05-2011“…We present XMM-Newton observations of three AGN taken as part of a hunt to find very heavily obscured Compton-thick AGN. For obscuring columns greater than…”
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Long-Term Variability in the Optical Spectrum of the Seyfert Galaxy NGC 2992
Published 09-04-2008“…The Astronomical Journal 135 (2008) 2048 New spectra of NGC 2992 from the Cerro Tololo Inter-American Observatory show that this nearby AGN has changed its…”
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A Monte Carlo Markov Chain based investigation of black hole spin in the active galaxy NGC3783
Published 19-06-2012“…The analysis of relativistically broadened X-ray spectral features from the inner accretion disk provides a powerful tool for measuring the spin of…”
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A Multi-Wavelength Study of the Nature of Type 1.8/1.9 Seyfert Galaxies
Published 13-10-2010“…We focus on determining the underlying physical cause of a Seyfert galaxy's appearance as type a 1.8 or 1.9. Are these "intermediate" Seyfert types typical…”
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Probing Relativistic Astrophysics Around SMBHs: The Suzaku AGN Spin Survey
Published 30-11-2011“…In addition to providing vital clues as to the formation and evolution of black holes, the spin of black holes may be an important energy source in the…”
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13
Modeling the Outflow in the Narrow-Line Region of Markarian 573:Biconical Illumination of a Gaseous Disk
Published 09-06-2010“…We present a study of the outflowing ionized gas in the resolved narrow-line region (NLR) of the Seyfert 2 galaxy Mrk 573, and its interaction with an in- ner…”
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Intrinsic Absorption Properties in Active Galaxies Observed with the Far Ultraviolet Spectroscopic Explorer
Published 01-07-2008“…In a continuing survey of active galactic nuclei observed by the Far Ultraviolet Spectroscopic Explorer, we provide a deeper analysis of intrinsic absorption…”
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Physical Conditions in the Inner Narrow Line Region of the Seyfert 2 Galaxy Markarian 573
Published 25-03-2009“…Astrophys.J.698:106-114,2009 We have examined the physical conditions within a bright emission-line knot in the inner narrow-line region (NLR) of the Seyfert 2…”
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16
Joint Ha and X-Ray Observations of Massive X-Ray Binaries. III. The Be X-Ray Binaries HDE 245770 = A0535+26 and X Persei
Published in The Astrophysical journal (10-05-2007)“…We present results from an Ha monitoring campaign of the Be X-ray binary systems HDE 245770 = A0535+26 and X Per. We use the Ha equivalent widths together with…”
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17
Joint H-alpha and X-Ray Observations of Massive X-Ray Binaries. III. The Be X-ray Binaries HDE 245770 = A 0535+26 and X Persei
Published 12-02-2007“…Astrophys.J.660:1398-1408,2007 We present results from an H-alpha monitoring campaign of the Be X-ray binary systems HDE 245770 = A 0535+26 and X Per. We use…”
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