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LSC 2366
Get PDFAudio recording of LSC 2366 presented by Landon Brady Saunders. The date of creation is estimated
Weldy, Margaret Alcestis (SC 2366)
Get PDFFinding aid only for Manuscripts Small Collection 2366. George Dennison Prentice, Editor of the Louisville Journal, 1830-1869 by Margaret Weldy, a thesis submitted in partial fulfillment of the requirements for the Master of Science degree, Columbia University, New York, New York, 1929
VARIABLE-STARS IN THE IRREGULAR GALAXY NGC-2366 (DDO-42)
No full textObservations of the resolved stars in the Irregular galaxy NGC 2366, obtained over the ten year period from March 1984 to March 1994, are presented. Thirty separate epochs were used to search for variable stars, and a total of 13 were found, of which 6 have characteristic Cepheid light curves and colors, After correction for galactic extinction these Cepheids yield a distance modulus, m-M=27.68 +/- 0.20. This corresponds to a distance of 3.44 Mpc which places NGC 2366 in the M81 Group, as has always been assumed. (C) 1995 American Astronomical Society.</p
Going Beyond Counting First Authors in Author Co-citation Analysis
Get PDFThe 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
Formalità per la convocazione (dell'assemblea di s.p.a.: art. 2366 c.c.)
No full textSi tratta del commento all'art. 2366 c.c. e quindi alla disciplina della convocazione dell'assemblea della s.p.a.; gli ultimi §§ del commento sono dedicati alla s.p.a. quotat
VARIABLE-STARS IN THE IRREGULAR GALAXY NGC-2366 (DDO-42)
No full textObservations of the resolved stars in the Irregular galaxy NGC 2366, obtained over the ten year period from March 1984 to March 1994, are presented. Thirty separate epochs were used to search for variable stars, and a total of 13 were found, of which 6 have characteristic Cepheid light curves and colors, After correction for galactic extinction these Cepheids yield a distance modulus, m-M=27.68 +/- 0.20. This corresponds to a distance of 3.44 Mpc which places NGC 2366 in the M81 Group, as has always been assumed. (C) 1995 American Astronomical Society
Block Card 2366 S. Byrne Road
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: Pyrofax Bottled Gas - Ohio - Toledo | commercial buildings | 2366 S. Byrne Road (Toledo, Ohio) | South Toledo Area (Toledo, Ohio
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