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相关论文: Supernova-Driven Outflows in NGC 7552: A Compariso…

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We obtained medium-resolution ultraviolet (UV) spectra between 1150 and 1450 Angstroms of the four UV-bright, infrared (IR)-luminous starburst galaxies IRAS F08339+6517, NGC 3256, NGC 6090, and NGC 7552 using the Cosmic Origins Spectrograph…

宇宙学与河外天体物理 · 物理学 2015-06-16 Claus Leitherer , Rupali Chandar , Christy Tremonti , Aida Wofford , Daniel Schaerer

We present new red optical spectra of V592 Cas aimed at exploring the properties of the outflow of this system in a spectral region where the underlying white dwarf and the accretion disk do not contribute significantly to the observed…

天体物理学 · 物理学 2009-11-13 S. Kafka , D. W. Hoard , R. K. Honeycutt , C. P. Deliyannis

Galactic outflows provide important feedback effects to regulate the evolution of host galaxies. Two primary diagnostics of outflows are broad and/or blueshifted emission and absorption lines. Even though well-established methods exist to…

The presence of broad wings in the H$\alpha$ line is commonly used as a diagnostic of the presence and properties of galactic winds from star-forming galaxies. However, the accuracy of this approach has not been subjected to extensive…

星系天体物理 · 物理学 2026-05-29 Rongjun Huang , Aditi Vijayan , Mark R. Krumholz

Star formation feedback can drive large-scale, multi-phase galactic outflows. The dynamical and thermodynamical interaction between the hot and cooler phases is a prime focus of both observational and theoretical work. Here, we analyze…

星系天体物理 · 物理学 2025-08-11 Sebastian Lopez , Laura A. Lopez , Todd A. Thompson , Adam K. Leroy , Alberto D. Bolatto

Ultrafast outflows (UFOs) have recently been found in the spectra of a number of active galactic nuclei (AGN) and are strong candidates for driving AGN feedback. 1H0707-495 is a highly accreting narrow line Seyfert 1 and the second most…

高能天体物理现象 · 物理学 2018-09-05 P. Kosec , D. J. K. Buisson , M. L. Parker , C. Pinto , A. C. Fabian , D. J. Walton

In order to reveal the origin of the ultra-fast outflows (UFOs) that are frequently observed in active galactic nuclei (AGNs), we perform two-dimensional radiation hydrodynamics simulations of the line-driven disk winds, which are…

高能天体物理现象 · 物理学 2017-01-25 Mariko Nomura , Ken Ohsuga

High-velocity outflows from AGN are a well-known phenomena in terms of the Broad Absorption Lines seen in the UV/optical. More recently, similar, possibly related, outflows have been reported in the X-ray. The most extreme example is seen…

天体物理学 · 物理学 2009-11-10 Paul T. O'Brien , James N. Reeves , Chris Simpson , Martin J. Ward

We have obtained detailed imaging Fabry-Perot observations of the nearby galaxy M82, in order to understand the physical association between the high-velocity outflow and the starburst nucleus. The observed velocities of the emitting gas in…

天体物理学 · 物理学 2010-01-07 P. L. Shopbell , J. Bland-Hawthorn

We present a unified picture of outflowing gas from the X-ray binary system Hercules X-1/HZ Herculis. We suggest that the outflowing gas (a wind) causes UV emission seen in mid-eclipse, narrow UV absorption lines, and broad UV P Cygni…

天体物理学 · 物理学 2009-11-07 Bram Boroson , Tim Kallman , Saeqa Dil Vrtilek

BOSS-EUVLG1 is the most ultraviolet (UV) and Ly$\alpha$ luminous galaxy detected so far in the Universe, going through a very active starburst phase, and forming stars at a rate (SFR) of 955 $\pm$ 118 M$_{\odot}$ yr$^{-1}$. We report the…

星系天体物理 · 物理学 2021-04-13 J. Álvarez-Márquez , R. Marques-Chaves , L. Colina , I. Pérez-Fournon

We present constraints on the molecular outflows in a sample of five Hyper-Luminous Infrared Galaxies using Herschel observations of the OH doublet at 119 {\mu}m. We have detected the OH doublet in three cases: one purely in emission and…

星系天体物理 · 物理学 2016-07-27 D. Calderón , F. E. Bauer , S. Veilleux , J. Graciá-Carpio , E. Sturm , P. Lira , S. Schulze , S. Kim

We show that the starburst-driven outflow in the peculiar galaxy NGC 2782 forms a well-defined collimated bubble which has an extent of $\sim$ 1 kpc and a closed shell at its edge, as seen in H$\alpha$, [O III], and 5 GHz radio continuum.…

天体物理学 · 物理学 2009-10-30 Shardha Jogee , Jeffrey D. P. Kenney , Beverly J. Smith

We observed the quasar PG1211+143 using the Cosmic Origins Spectrograph on the Hubble Space Telescope in April 2015 as part of a joint campaign with the Chandra X-ray Observatory and the Jansky Very Large Array. Our ultraviolet spectra…

The velocity structure imprinted in the H{\alpha} emission line profiles contains valuable information about galactic outflows. Using a set of high-resolution zoom-in cosmological simulations of galaxies at z=2, we generate H{\alpha}…

We investigate the multi-phase structure of gas flows in galaxies. We study 80 galaxies during the epoch of peak star formation ($1.4\leq z\leq2.7$) using data from Keck/LRIS and VLT/KMOS. Our analysis provides a simultaneous probe of…

We present discovery spectra of a sample of eight lensed galaxies at high redshift, 3.7<z<5.2, selected by their red colors in the fields of four massive clusters: A1689, A2219, A2390, and AC114. Metal absorption lines are detected and…

天体物理学 · 物理学 2009-11-07 Brenda Frye , Tom Broadhurst , Narciso Benitez

We present new Hubble Space Telescope Cosmic Origins Spectrograph far-ultraviolet (far-UV) spectroscopy and Keck Echellete optical spectroscopy of 11 ultraluminous infrared galaxies (ULIRGs), a rare population of local galaxies experiencing…

星系天体物理 · 物理学 2015-06-23 Crystal L. Martin , Mark Dijkstra , Alaina Henry , Kurt T. Soto , Charles W. Danforth , Joseph Wong

We present Adaptive Optics assisted near-IR integral field spectroscopic observations of a luminous quasar at $z = 2.4$, previously observed as the first known example at high redshift of large scale quasar-driven outflow quenching star…

星系天体物理 · 物理学 2017-03-22 R. J. Williams , R. Maiolino , Y. Krongold , S. Carniani , G. Cresci , F. Mannucci , A. Marconi

Spectropolarimetry results for the starburst galaxy M82 are presented. The optical emission lines of the filaments in the energetic outflow ("superwind") from the nuclear starburst region of M82 are substantially polarized. The H-alpha…

宇宙学与河外天体物理 · 物理学 2015-05-20 Michitoshi Yoshida , Koji S. Kawabata , Youichi Ohyama
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