Results 21 to 30 of about 68,770 (231)

Long-slit spectroscopy of starburst galaxies

open access: yesThe Astrophysical Journal, 1988
We present high-resolution, long-slit spectra of nine optically bright nuclear star-burst galaxies (SBGs) selected from the sample of Balzano from which we measure line strengths, line widths, and velocity profiles along the slit in the Hα, [N II], and [S II] emission lines.
Richard A. Shaw, Michael M. De Robertis
openaire   +1 more source

Spectroscopy of Luminous Infrared Galaxies [PDF]

open access: yesSymposium - International Astronomical Union, 1999
A review of recent optical and infrared spectroscopic results on luminous infrared galaxies is presented. The main emphasis is on the ultraluminous objects. Possible correlations with infrared luminosity are identified. These results are used to constrain the nature of the dominant energy source in luminous infrared galaxies, and to test whether these ...
openaire   +1 more source

Spectroscopy of the galaxy components of N and Seyfert galaxies [PDF]

open access: yesPublications of the Astronomical Society of the Pacific, 1987
Nuclear and off-nuclear spectra of nine active galaxies are presented. The sample consists of four Seyfert galaxies, two N galaxies, one Seyfert radio galaxy, and one liner/Seyfert 2 galaxy. All of the objects show continuum emission off the nucleus. Four clearly show absorption features from a stellar population.
Todd A. Boroson, J. B. Oke
openaire   +1 more source

CLASSY. VI. The Density, Structure, and Size of Absorption-line Outflows in Starburst Galaxies

open access: yesThe Astrophysical Journal, 2023
Galaxy formation and evolution are regulated by the feedback from galactic winds. Absorption lines provide the most widely available probe of winds.
Xinfeng Xu   +14 more
doaj   +1 more source

On-axis spectroscopy of the host galaxies of 20 optically luminous quasars at z~0.3 [PDF]

open access: yes, 2006
We present the analysis of a sample of 20 bright low-redshift quasars ...
Courbin, F.   +6 more
core   +4 more sources

Minor Mergers Are Not Enough: The Importance of Major Mergers during Brightest Cluster Galaxy Assembly

open access: yesThe Astrophysical Journal Supplement Series, 2023
We investigate the roles of major and minor mergers during brightest cluster galaxy (BCG) assembly using surface brightness profiles, line indices, and fundamental plane relations.
Matthias Kluge, Ralf Bender
doaj   +1 more source

JHK Spectra of the z=2.39 Radio Galaxy 53W002 [PDF]

open access: yes, 2001
We present low-resolution, near-IR JHK spectra of the weak z=2.39 radio galaxy 53W002, obtained with the OH-airglow Suppressor spectrograph (OHS) and Cooled Infrared Spectrograph and Camera for OHS (CISCO) on the Subaru Telescope.
Harashima, T.   +9 more
core   +2 more sources

Slit and integral-field optical spectroscopy of the enigmatic quasar HE0450-2958 [PDF]

open access: yes, 2008
Interest in the quasar HE0450-2958 arose following the publication of the non-detection of its expected massive host, leading to various interpretations. This article investigates the gaseous and stellar contents of the system through additional VLT/FORS
Baldwin   +21 more
core   +1 more source

Spectroscopy of Three SBS Galaxies [PDF]

open access: yesSymposium - International Astronomical Union, 1996
Three galaxies from Second Byurakan Sky Survey have been studied. The spectra of these galaxies were obtained at 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. For these objects line widths and emission line ratios were measured and ionization mechanism and chemical abundances were determined.
openaire   +1 more source

The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies

open access: yesThe Astrophysical Journal, 2023
The Dark Energy Spectroscopic Instrument (DESI) Survey has obtained a set of spectroscopic measurements of galaxies to validate the final survey design and target selections.
Ting-Wen Lan   +81 more
doaj   +1 more source

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