1,725,622 research outputs found
Astronomische Nachrichten, Nos 3505-3512
No full textAstronomische Nachrichten, Nos 3505-3512. In: Bulletin astronomique, tome 16, 1899. pp. 445-448
Salt Lake Route Engine #3505
No full textImage shows a large Salt Lake Route locomotive, Engine #3505, parked at a Salt Lake City railroad yard
3505 Turtle Creek, Dallas, ca. 1962
No full text3505 Turtle Creek, Dallas, ca. 1962https://mavmatrix.uta.edu/specialcollections_squirehaskinsphotography/5156/thumbnail.jp
Denver & Rio Grande Western (DRGW) 3505
No full textA photograph print showing Denver & Rio Grande Western (DRGW) 3505, 2-8-8-2, on freight train, Denver, CO
Block Card 3505 Greengate Drive
No full textThis image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: 3505 Greengate Drive (Toledo, Ohio) | duplexes | Byrne Way Subdivision (Toledo, Ohio) | South Toledo Area (Toledo, Ohio) | Modern Colonial Styl
GASS 3505: The prototype of HI-excess, passive galaxies
No full textWe present our multiwavelength analysis of a prototype H I-excess galaxy, GASS 3505, selected based on having a large gas content (M_{H I} = 10^{9.9} M☉) compared to its little associated star formation activity (̃0.1 M☉ yr-1) in the GALEX Arecibo SDSS Survey (GASS). Very Large Array observations show that the H I in GASS 3505 is distributed in a regularly rotating, extended (̃50 kpc radius) gas ring. In the SDSS optical image GASS 3505 appears as a bulge-dominated galaxy, however deep optical imaging reveals low surface brightness (≳25 mag arcsec-2) stellar emission around the central bulge. Direct evidence for accretion is detected in form of an extended (̃60 kpc) stellar stream, showing that GASS 3505 has experienced a minor merger in the recent past. We investigate the possibility that the H I ring in GASS 3505 was accreted in such a merger event using N-body and smoothed particle hydrodynamic simulations. The best model that reproduces the general properties (i.e. gas distribution and kinematics, stellar morphology) of the galaxy involves a merger between the central bulge and a gas-rich (M⋆ = 109 M☉ and M_{H I}/M⋆ = 10) disc galaxy. However, small discrepancies in the observed and modelled properties could suggest that other sources of gas have to be involved in the build-up of the gas reservoir. This work is the first step towards a larger program to investigate the physical mechanisms that drive the large scatter in the gas scaling relations of nearby galaxies
Block Card 3505 Burton Avenue
No full textThis image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: dwelling | 3505 Burton Avenue (Toledo, Ohio) | Bungalow Style | Craftsman Style | Almeda Heights Second Addition (Toledo, Ohio) | Willys Park area (Toledo, Ohio) | West Toledo (Toledo, Ohio
- …
