Results 51 to 60 of about 859,267 (172)
High-Resolution Mid-Infrared Imaging of Infrared-Luminous Starburst Galaxies [PDF]
Observations for seven infrared-luminous starburst galaxies are reported in the mid-infrared from 8 to 18 μm using the Keck telescopes with spatial resolution approaching the diffraction limit.
Becklin, E. E. +9 more
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A Complete 16 μm Selected Galaxy Sample at z ∼ 1. II. Morphological Analysis
We present a morphological analysis of the 16 μ m flux-density-limited galaxy sample at 0.8 < z < 1.3 from Huang et al. (2021). At the targeted redshift, the 16 μ m emission corresponds to the polycyclic aromatic hydrocarbon feature from intense star ...
Piaoran Liang +4 more
doaj +1 more source
An Hα Impression of Lyα Galaxies at z ≃ 6 with Deep JWST/NIRCam Imaging
We present a study of seven spectroscopically confirmed (Ly α -emitting) galaxies at redshift z ≃ 6 using the JWST/NIRCam imaging data. These galaxies, with a wide range of Ly α luminosities, were recently observed in a series of NIRCam broad and medium ...
Yuanhang Ning +5 more
doaj +1 more source
Morphology of luminous IRAS galaxies: Summary talk [PDF]
The author discusses the morphology of luminous Infrared Astronomy Satellite (IRAS) galaxies.
Becklin, E. E.
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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
Probing extreme black‐hole outflows on short timescales via high spectral‐resolution x‐ray imagers
Abstract We investigate outflows and the physics of super‐Eddington versus sub‐Eddington regimes in black hole systems. Our focus is on prospective science using next‐generation high‐resolution soft x‐ray instruments. We highlight the properties of black hole ultraluminous x‐ray source (ULX) systems in particular. Owing to scale invariance in accreting
C. Pinto +9 more
wiley +1 more source
Characterising Nearby Luminous Infrared Galaxies [PDF]
Luminous InfraRed Galaxies (LIRGs) in the local universe are known to be highly interacting galaxies with strong star-formation in obscured environments.
Ramphul, R., Vaisanen, P., Van der Heyden, K. (5304589) +1 more
core +1 more source
Infrared-luminous galaxies are important sites of stellar and black hole mass assembly at most redshifts. Their luminosities are often estimated by fitting spectral energy distribution (SED) models to near- to far-infrared data, but the dependence of ...
Duncan Farrah +25 more
doaj +1 more source
Abstract We present James Webb Space Telescope observations of the globular cluster NGC 6397 and use them to extend to infrared wavelengths the characterization of the cluster's entire white dwarf (WD) cooling sequence (CS). The data allows us to probe fundamental astrophysical WD properties and to search for evidence in their colors for (or against ...
L. R. Bedin +11 more
wiley +1 more source
The clustering of dark matter, haloes & galaxies [PDF]
In this thesis I study the spatial distribution of galaxies, haloes and dark matter particles using a suite of state-of-art cosmological N-body simulations of the growth structure in the Universe.
Angulo de la Fuente, Raúl Esteban
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