1,728,653 research outputs found
A new narrow-line Seyfert 1 galaxy: RX J1236.9+2656
No full textWe report identification of a narrow-line Seyfert 1 galaxy RX J1236.9+2656. X-ray emission from the NLS1 galaxy undergoes long-term variability with 0.1-2.0 keV flux changing by a factor of ∼ 2 within ∼3. The ROSAT PSPC spectrum of RX J1236.9+2656 is well represented by a power-law of Γx=3.7+0.5−0.3 absorbed by matter in our own Galaxy (NH=1.33×1020 cm−2). Intrinsic soft X-ray luminosity of the NLS1 galaxy is estimated to be ∼ 1.5×1013 erg s−1 in the energy band of 0.1-2.0keV. The optical spectrum of RX J1236.9+2656 is typical of NLS1 galaxies and shows narrow Balmer emission lines (1100 km s−1 < FWHM < 1700 km s−1) of Hβ, Hα, and forbidden lines of [O III] and [N II]. Fe II multiplets, usually present in optical spectra of NLS1 galaxies, are also detected in RX J1236.9+2656
A new narrow-line Seyfert 1 galaxy: RX J1236.9+2656
No full textWe report identification of a narrow-line Seyfert 1 galaxy RX J1236.9+2656. X-ray emission from the NLS1 galaxy undergoes long-term variability with 0.1-2.0 keV flux changing by a factor of ∼ 2 within ∼3. The ROSAT PSPC spectrum of RX J1236.9+2656 is well represented by a power-law of Γx=3.7+0.5−0.3 absorbed by matter in our own Galaxy (NH=1.33×1020 cm−2). Intrinsic soft X-ray luminosity of the NLS1 galaxy is estimated to be ∼ 1.5×1013 erg s−1 in the energy band of 0.1-2.0keV. The optical spectrum of RX J1236.9+2656 is typical of NLS1 galaxies and shows narrow Balmer emission lines (1100 km s−1 < FWHM < 1700 km s−1) of Hβ, Hα, and forbidden lines of [O III] and [N II]. Fe II multiplets, usually present in optical spectra of NLS1 galaxies, are also detected in RX J1236.9+2656
Block Card 2656 Overbrook 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: Split-Level Style | 2656 Overbrook Drive (Toledo, Ohio) | Dwelling | Arden Place Subdivision (Toledo, Ohio) | South Toledo Area (Toledo, Ohio
Block Card 2656 Wyndale 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: Dwelling | 2656 Wyndale Road (Toledo, Ohio) | Ranch houses | Maxwell Place Plat Two (Toledo, Ohio) | Deveaux Area (Toledo, Ohio) | West Toledo area (Toledo, Ohio
Block Card 2656 Juniper 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 | 2656 Juniper Drive (Toledo, Ohio) | Dwelling | Arden Place Subdivision (Toledo, Ohio) | South Toledo Area (Toledo, Ohio
McGown, Hattie Russ (SC 2656)
Full text linkFinding aid only for Manuscripts Small Collection 2656. Letter of Hattie (Mrs. Hugh) McGown, Bowling Green, Kentucky, to her sister Burlie Ellis, Richelieu, Kentucky. She reports on her husband’s work as a railroad switchman, the participation of her son Joe in a school play, and her progress in joining a new church. She also describes witnessing efforts to extract a car from a ditch on her family’s return from a visit to her father
Floor Statement on S. 2656 - Proposed Payroll Reform Tax Legislation
Full text linkWashington, D.C.
Date: October 5, 1971
Senator Edmund S. Muskie introduces S. 2656, a bill to reform the payroll tax.https://scarab.bates.edu/msp/1149/thumbnail.jp
J.A.M.I.E.
No full textJAMIE: Jurnal Abdi Masyarakat Ilmu Ekonomi merupakan jurnal publikasi hasil kegiatan pengabdian kepada masyarakat bidang ekonomi khususnya pada ilmu ekonomi, ilmu akuntansi, dan ilmu manajemen bertujuan melakukan perubahan perilaku masyarakat dalam pemanfaatan dan pemaksimalan sumber daya (SDM dan SDA) yang dimiliki untuk kesejahteraan.
http://jurnal.fem.uniba-bpn.ac.id/index.php/JAMIE/issue/view/jamiep-ISSN:2656-3517 | e-ISSN:2656-3908 | http://jurnal.fem.uniba-bpn.ac.id/index.php/JAMIE/issue/view/jami
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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