Results 91 to 100 of about 833,890 (231)
Over half of the far-infrared background light comes from galaxies at z ≥ 1.2 [PDF]
, 2009 Submillimetre surveys during the past decade have discovered a population of luminous, high-redshift, dusty starburst galaxies¹⁻⁸. In the redshift range 1 ≤ z ≤ 4, these massive submillimetre galaxies go through a phase characterized by optically ...
David Hughes, ITZIAR ARETXAGA MENDEZ
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Dense Ionized Outflow with Five Narrow Components in a Dust-obscured Galaxy
The Astrophysical JournalWe present our discovery of a complex ionized outflow in SDSS J101034.28+372514.7 (J1010+3725), a dust-obscured galaxy (DOG) at z = 0.282. The Sloan Digital Sky Survey optical spectrum of J1010+3725 shows five narrow components with one broad component ...
Taketo Yoshida +6 more
doaj +1 more source
The clustering and X-ray properties of faint galaxies [PDF]
, 1994 The clustering properties of faint (23 ≤ B ≤ 27) galaxies were investigated, with the aim of obtaining information about their redshift distribution, N(z), and therefore about the processes of galaxy evolution causing the steep rise in the galaxy number ...
Roche, Nathan, Roche, N
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Astronomy & AstrophysicsThe NIKA2 Cosmological Legacy Survey (N2CLS) is a large programme using the NIKA2 dual-band camera on the IRAM 30 m telescope. Its goal is to improve our understanding of the physics of distant Dusty Star Forming Galaxies (DSFGs) by carrying out deep ...
Ponthieu N. +56 more
doaj +1 more source
Normal Galaxies in the Infrared [PDF]
, 2007 This review addresses what can be learned from infrared observations about galaxies powered predominantly by star formation. Infrared techniques mostly probe the interstellar medium of galaxies, yielding physical and chemical information on the medium out of which stars form, which is in turn affected by those stars.
openaire +3 more sources
Low luminosity elliptical galaxies [PDF]
, 1998 Long-slit spectra for the photometric axes of a sample of 14 elliptical galaxies, predominantly low-luminosity ellipticals, in the Virgo cluster and in nearby groups, are studied to investigate the galaxy kinematical structure and stellar evolutionary ...
Halliday, Claire, Halliday, C.
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Near-infrared imaging of interacting galaxies
The Astrophysical Journal, 1990 Galaxy-galaxy interactions are known to cause dramatic changes in morphology and at the same time often induce large bursts of star formation activity. While optical images are sufficient to reveal the overall morphological peculiarities of these systems, they suffer from several problems, the greatest of which is obscuration by dust within the ...
H. A. Bushouse, M. W. Werner
openaire +1 more source
The physiology of survival: Space
Experimental Physiology, Volume 111, Issue 9, Page 3890-3894, 1 September 2026.
Damian M. Bailey, Angelique van Ombergen
wiley +1 more source
The QSO — Ultraluminous Infrared Galaxies Connection [PDF]
, 2001 For the past several years, our group has pursued a vigorous ground-based program aimed at understanding the nature of ultraluminous infrared galaxies. We recently published the results from a optical/near-infrared spectroscopic survey of a large statistically complete sample of ultraluminous infrared galaxies (the "IRAS 1-Jy sample").
Veilleux, S. +2 more
openaire +2 more sources
A complete redshift sample of galaxies [PDF]
, 1983 The role of complete redshift samples is discussed with particular attention focused on the need for new deeper and better controlled surveys for statistical clustering and dynamical studies.
Bean, A.J., Bean, Adrian John
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