Results 101 to 110 of about 2,538 (226)

Recent Star Formation in Very Luminous Infrared Galaxies [PDF]

open access: yes, 2001
Among star forming galaxies, a spectral combination of a strong Hdelta line in absorption and a moderate [OII] emission has been suggested to be a useful method to identify dusty starburst galaxies at any redshift, on the basis of optical data alone.
Bressan, A.   +2 more
openaire   +2 more sources

HST astrometry of the closest brown dwarfs‐II. Improved parameters and constraints on a third body

open access: yesAstronomische Nachrichten, Volume 345, Issue 1, January 2024.
Abstract Located at less than two pc away, Luhman 16 AB (WISE J104915.57‐531906.1) is the closest pair of brown dwarfs and the third closest “stellar” system to Earth. An exoplanet candidate in the Luhman 16 binary system was reported in 2017 based on a weak astrometric signature in the analysis of 12 HST epochs.
L. R. Bedin   +7 more
wiley   +1 more source

The Hidden H I-Massive Luminous Infrared Galaxy HIZOA J0836–43: Inside-Out Galaxy Formation [PDF]

open access: yes, 2008
HIZOA J0836–43 is an extreme gas-rich (MH I = 7.5 × 10^10 M☉) disk galaxy which lies hidden behind the strongly obscuring Vela region of the Milky Way.
Koribalski, B. S.   +8 more
core  

Obscured AGN at z < 1.5: X-Ray to Far-infrared SEDs and Host Galaxy Morphologies in the GOODS Fields

open access: yesThe Astrophysical Journal
We present an analysis of spectral energy distributions (SEDs), galaxy light profiles, and visual morphological classifications for 194 X-ray luminous active galactic nuclei (AGN) (intrinsic absorption-corrected $\mathrm{log}({L}_{{\rm{X}},0.5-7\,{\rm ...
William W.H. Jarvis   +11 more
doaj   +1 more source

Halfway to the Peak: Kinematic Signatures of Stable Rotating Disks in Luminous Infrared Galaxies at z = 0.5–0.6

open access: yesThe Astrophysical Journal
We present a kinematic study of six IR-luminous galaxies observed with the Mid-infrared Instrument Medium-resolution Spectrometer (MIRI/MRS) on board JWST.
Miriam Eleazer   +15 more
doaj   +1 more source

Rest-Frame Mid-Infrared Detection of an Extremely Luminous Lyman Break Galaxy with the Spitzer Infrared Spectrograph (IRS) [PDF]

open access: yes, 2004
We present the first rest-frame of approximately 4 microns detection of a Lyman break galaxy. The data were obtained using the 16 microns imaging capability of the Spitzer Infrared Spectrograph.
Grillmair, C.   +17 more
core  

UGC 2369S: A Kiloparsec-scale Triple Merger Candidate Identified in a Nearby Luminous Infrared Galaxy

open access: yesThe Astrophysical Journal
We present high-spatial-resolution (≲1 $\mathop{.}\limits{^{\prime\prime} }$ 0), multiwavelength observations of UGC 2369S, a nearby luminous infrared galaxy showing three distinct cores separated on kiloparsec scales in near-infrared (NIR) imaging with ...
Yuanze Ding   +14 more
doaj   +1 more source

LWS spectroscopy of the luminous blue compact galaxy Haro 11 [PDF]

open access: yes, 2000
We present the results of far infrared (FIR) spectroscopy of the luminous blue compact galaxy (BCG) Hare 11 (ESO 350-IG38) obtained with the Long Wavelength Spectrometer (LWS) on the Infrared Space Observatory (ISO) in low resolution mode.
Masegosa, J   +3 more
core  

Adaptive optics imaging and optical spectroscopy of a multiple merger in a luminous infrared galaxy [PDF]

open access: yes, 2008
We present near-infrared (NIR) adaptive optics imaging obtained with VLT/NACO and optical spectroscopy from the Southern African Large Telescope (SALT) of a luminous infrared galaxy (LIRG) IRAS 19115-2124.
Romero-Colmenero, E.   +35 more
core   +1 more source

On the Very Bright Dropouts Selected Using the James Webb Space Telescope NIRCam Instrument

open access: yesThe Astrophysical Journal
The selection of candidate high-redshift galaxies using the dropout technique targeting the Lyman-break signature sometimes yields very bright objects that are too luminous to be easily explained if they are indeed at the expected redshifts.
Bangzheng Sun, Haojing Yan
doaj   +1 more source

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