Results 151 to 160 of about 411 (185)
Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn
Fujimoto S +45 more
europepmc +1 more source
A Faint Progenitor System for the Faint Supernova 2024vjm
Zimmerman E +69 more
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A Network Approach for the Accurate Characterization of Water Lines Observable in Astronomical Masers and Extragalactic Environments. [PDF]
Ubachs W +4 more
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A detailed analysis of the Czernik 38 cluster and its associated tidal tail, utilizing Gaia DR3 and 2MASS. [PDF]
Ahmed NM.
europepmc +1 more source
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Resolving the hot and ionized Universe through the Sunyaev-Zeldovich effect. [PDF]
Di Mascolo L +25 more
europepmc +1 more source
Infrared bands of neutral gas-phase carbon clusters in a broad spectral range.
Ferrari P, Lemmens AK, Redlich B.
europepmc +1 more source
Environmental dependence of local luminous infrared galaxies [PDF]
14 pages, 17 figures. To appear in A&A. Paper with high resolution figures is available at http://astro.kias.re.kr/~hshwang/doc/ms_hwang_lirg ...
Ho Seong Hwang, Hyung Mok Lee
exaly +3 more sources
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Annual Review of Astronomy and Astrophysics, 1996
▪ Abstract At luminosities above 1011 [Formula: see text], infrared galaxies become the dominant population of extragalactic objects in the local Universe (z ≲ 0.3), being more numerous than optically selected starburst and Seyfert galaxies and quasi-stellar objects at comparable bolometric luminosity.
D. B. Sanders, I. F. Mirabel
openaire +1 more source
▪ Abstract At luminosities above 1011 [Formula: see text], infrared galaxies become the dominant population of extragalactic objects in the local Universe (z ≲ 0.3), being more numerous than optically selected starburst and Seyfert galaxies and quasi-stellar objects at comparable bolometric luminosity.
D. B. Sanders, I. F. Mirabel
openaire +1 more source
Evolution of the ISM in luminous infrared galaxies [PDF]
Aims. Molecules that trace the high-density regions of the interstellar medium may be used to evaluate the changing physical and chemical environment during the ongoing nuclear activity in (ultra-) luminous infrared galaxies (ULIRGs).Methods. The changing ratios of the HCN (1-0), HNC (1-0), HCO(+) (1-0), CN (1-0) and CN (2-1), and CS (3-2) transitions ...
M Spaans
exaly +3 more sources

