1,724,884 research outputs found
Block Card 4710 Alfred Street
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 | 4710 Alfred Street (Toledo, Ohio) | Ranch Style | North Toledo (Toledo, Ohio) | Willys Park area (Toledo, Ohio) | Alfred Bailey Addition (Toledo, Ohio
Block Card 4710 Oakridge 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: Ranch houses | Dwelling | 4710 Oakridge Drive (Toledo, Ohio) | Secor Woods Addition (Toledo, Ohio) | Trilby Area (Toledo, Ohio)) | West Toledo Area (Toledo, Ohio
Block Card 4710 Stengel 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: Cape Cod Style | 4710 Stengel Avenue (Toledo, Ohio) | Dwelling | South Toledo Area (Toledo, Ohio
Block Card 4710 Monac 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: Cape Cod Style | 4710 Monac Drive (Toledo, Ohio) | Dwelling | Greenbush Knolls Addition (Toledo, Ohio) | Trilby Area (Toledo, Ohio)
An hi study of the nearby dwarf galaxy ic 4710
Get PDF>Magister Scientiae - MScThis work aims to study the dark matter content of the nearby (7.38 Mpc) dwarf
galaxy IC 4710 using the HI line observations from the Australia Telescope
Compact Array (ATCA). We produce the rst interferometric maps of the
galaxy HI distribution and dynamics and use these maps to measure important
quantities such as total HI mass, velocity width, and size. We create a dynamical
model of the galaxy using a three-dimensional modeling technique. The rotation
curve was obtained by tting a 3D tilted ring model to the HI data cube of
galaxy IC 4710. The dynamical modeling of IC 4710 is being done for the rst
time. We compare the model to the data cube to check for accuracy and found
that they are in good agreement; this shows that the results are reliable. The
obtained rotation curve is rising steeply until it reaches the maximum rotation
velocity of 24.6 km s1 at a radius of 100 arcsec
An hi study of the nearby dwarf galaxy ic 4710
No full text>Magister Scientiae - MScThis work aims to study the dark matter content of the nearby (7.38 Mpc) dwarf
galaxy IC 4710 using the HI line observations from the Australia Telescope
Compact Array (ATCA). We produce the rst interferometric maps of the
galaxy HI distribution and dynamics and use these maps to measure important
quantities such as total HI mass, velocity width, and size. We create a dynamical
model of the galaxy using a three-dimensional modeling technique. The rotation
curve was obtained by tting a 3D tilted ring model to the HI data cube of
galaxy IC 4710. The dynamical modeling of IC 4710 is being done for the rst
time. We compare the model to the data cube to check for accuracy and found
that they are in good agreement; this shows that the results are reliable. The
obtained rotation curve is rising steeply until it reaches the maximum rotation
velocity of 24.6 km s1 at a radius of 100 arcsec
CDFS 4710: Economic and Social Contexts of Individuals and Families
No full textThe first chapter from an Open Educational Resource textbook created for MTSU's course CDFS 4710: Economic and Social Contexts of Individuals and Families
Linked collectors and determiners for: ANM Zoological vertebrate collection.
No full textNatural history specimen data linked to collectors and determiners held within, "ANM Zoological vertebrate collection". Claims or attributions were made on Bionomia by volunteer Scribes, <a href="http://bionomia.net/dataset/0dac68d7-afad-4710-a871-3233ffe0c0d3">https://bionomia.net/dataset/0dac68d7-afad-4710-a871-3233ffe0c0d3</a> using specimen data from the dataset aggregated by the Global Biodiversity Information Facility, <a href="https://gbif.org/dataset/0dac68d7-afad-4710-a871-3233ffe0c0d3">https://gbif.org/dataset/0dac68d7-afad-4710-a871-3233ffe0c0d3</a>. Formatted as a Frictionless Data package
Current star formation in S0 galaxies: NGC 4710
Get PDFElliptical (E) and lenticular (S0) galaxies lack the substantial interstellar medium (ISM) found in the star-forming spiral galaxies. However, significant numbers of E and S0 galaxies are known to contain detectable amounts of interstellar matter (e.g., Jura 1988). Thus, it is worth investigating whether these galaxies are currently able to form stars from their ISM, or whether they should be consigned to the dustbin of inert objects (Thronson and Bally 1987). The results strongly imply that current star formation is responsible for NGC 4710's far infrared and radio continuum properties. If this is indeed the case, then one expects this star formation to be fueled by molecular gas, which is presumably dominated by H2 and can be traced by the CO-12 J=1 to 0 line. Both Kenney and Young (1988) and Sage and Wrobel (1989) have detected such an emission line from NGC 4710, and infer the presence of more than 10(exp 8) solar mass of H2. The origin of the molecular gas in NGC 4710 remains a mystery. The galaxy is very deficient in HI (Kenney and Young, in preparation), suggesting that it originally was a spiral galaxy from which the outer, mainly atomic, gas was stripped by the ram pressure of the Virgo Cluster's intracluster medium, leaving only a central interstellar medium (ISM) rich in molecular gas. Alternatively, the CO may have originated via stellar mass loss with subsequent cooling, cooling flows, or capture from a gas-rich companion. Information on the morphology and kinematics of the CO can be compared with that of the galaxy's other gases and stars to distinguish among these various possible origins for the molecular gas. Major axis CO mapping with single dishes indicate an unresolved source. Thus, a millimeter array is currently being used to image NGC 4710 in CO to provide the needed morphological and kinematical data
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