1,725,156 research outputs found
Block Card 3359 Bishop 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: Carpenter Gothic Style | 3359 Bishop Street (Toledo, Ohio) | Dwelling | Clifton Park Addition | Auburndale Area (Toledo, Ohio
Block Card 3359 Lagrange 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 | 3359 Lagrange Street (Toledo, Ohio) | Curved Bay Folk House | North Toledo (Toledo, Ohio) | Lagrange Area (Toledo, Ohio) | Doppkes St. Adalbert Additio
Block Card 3359 Grayling Place
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 | 3359 Grayling Place (Toledo, Ohio) | Dwelling | Grayling Place Addition (Toledo, Ohio) | Trilby Area (Toledo, Ohio)
Grise, George Calvin, 1918-1960 (SC 3359)
Full text linkFinding aid only for Manuscripts Small Collection 3359. Letters and cards to WKU faculty member Frances Richards and her parents, and writings of George C. Grise. The WKU graduate, English professor at Austin Peay State University, and author thanks the Richards for gifts, including a loom, and describes his life in the country near Lewisburg, Kentucky. He sends Frances Richards notices regarding the publication of his 1956 book Life With Hezzie and a 1960 writer’s workshop at Austin Peay. Includes an essay about editing WKU’s College Heights Herald newspaper, and a published article about school discipline stories. Also includes clippings about Grise and an acknowledgment of sympathy card from his family after his death in an auto accident
Orthodox religious beliefs and anti-semitism: A replication of Glock and Stark in the Netherlands
Full text linkContains fulltext :
3359.pdf (Publisher’s version ) (Open Access
Episodicity in accretion-ejection processes associated with IRAS 15398-3359
Full text linkContext. The protostar IRAS 15398-3359 is associated with a bipolar molecular outflow ejected in an nearly northeast-southwest (NE–SW) direction, which has been extensively studied. Previous episodic accretion events have been suggested by this source. Furthermore, the analysis of the morphology and kinematics of the molecular outflow revealed the presence of four 12CO (2–1) bipolar elliptical shock-like structures identified in both lobes. These structures seem to trace different ejections inclined ~10° from each other on the plane of the sky. This led to the hypothesis that the outflow axis likely precesses and launches material episodically.
Aims. Since several authors reached the conclusion of the same episodicity scenario by independent observations, IRAS 15398-3359 has become an ideal target to empirically analyze the relationship between accretion and ejection processes.
Methods. We analyzed ALMA archive observations in Band 6, revealing the presence of low-velocity (<3.5 km s−1) emission from the 12CO (2−1) line to the south and north of the protostar. We studied the morphology and kinematics of the gas; our study seems to support the hypothesis of a precessing episodic outflow.
Results. The ALMA observations reveal a north–south (N–S) outflow most likely associated with the IRAS 15398-3359 protostellar system. This outflow could be older than the well-studied NE–SW outflow. The orientation of the N–S outflow is 50°–60° on the plane of the sky away from that of the NE–SW outflow. We also analyzed the spectral energy distribution of a far away young star and preliminarily discard it as the driver of the SE outflow remnants.
Conclusions. The new observations support the hypothesis of strong episodic accretion-ejection events in IRAS 15398-3359, accompanied by dramatic changes in the orientation of its ejection axis, implying that all the outflows in the region may have been driven by the same protostar
Going Beyond Counting First Authors in Author Co-citation Analysis
Full text linkThe present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation
counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings
are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that
only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into
account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed
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