Setting off from the presupposition that the library collections of monastery libraries are of immense cultural value, and can therefore be considered cultural good and part of Croatian written heritage, the paper discussed the need for a systematic approach to its protection, both on the operative level, in libraries themselves, and on the strategic level, by the authorities and other relevant institutions in the Republic of Croatia. Organizational prerequisites for the preservation of library collections in monastery librariesĭirectory of Open Access Journals (Sweden)įull Text Available The aim of the paper is to investigate the preservation of written heritage in monastery libraries from legislative, institutional and organizational perspectives, and establish the necessary organizational prerequisites for improvement. This book encompasses different areas of collection management and cover topics, such as: collection management in the organizational context collection development policies selection principles and resources budget management and more. The management of information resources in libraries is of greater importance in the digital world. Managing information resources in libraries collection management in theory and practice
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National Archives and Records Administration — MCMD serves as a descriptive catalog for the Presidential Libraries museum collections, and also supports a full range of museum collections management processes. The outflow properties, such as the mass outflow rate (∼0.1 M ⊙ yr −1), the outflow kinetic power (∼5.2 × 10 −4% L bol), and the mass loading factor (∼0.12), point toward a scenario where the measured feedback is not strong and has a low impact on the evolution of galaxies in general.Presidential Libraries Museum Collection Management Database The observed emission-line ratios are best reproduced by photoionization models when compared to shock ionization, indicating that radiation from the young stellar population is dominant and seems to be a consequence of a continuous star-formation activity instead of a “bursty” event. By modeling the broadband spectra with spectral energy distribution fitting and obtaining the star-formation histories of the sample, we observe a small decrease in SFR between 100 and 10 Myr in galaxies when the outflow H α luminosity contribution is increased, indicating that the feedback somewhat inhibits the star formation within these timescales. This interpretation is in agreement with the correlation between the observed star-formation rate (SFR) surface density (Σ SFR) and the second-component velocity dispersion ( σ 2nd), expected when tracing the feedback component. We measure the emission-line spectra by fitting a double-component profile, with the second and broader component related to the outflowing gas. We characterize the ionized gas outflows in 15 low-redshift star-forming galaxies, a Valparaíso ALMA/APEX Line Emission Survey (VALES) subsample, using MUSE integral field spectroscopy and GAMA photometric broadband data. School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, PR ChinaĬePIA, Departamento de Astronomía, Universidad de Concepción, Casilla 160-C, Concepción, Chile Gran Bretaña 1111, Valparaíso, ChileĬAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, PR China Instituto de Física y Astronomía, Universidad de Valparaíso, Avda. Hughes 2 ,3 ,4 ,5, Médéric Boquien 1, Eduardo Ibar 3, Sébastien Viaene 6, ⋆, Roger Leiton 7 and Yongquan Xue 4 ,5Ĭentro de Astronomía (CITEVA), Universidad de Antofagasta, Avenida Angamos 601, Antofagasta, ChileĮ-mail: Academy of Sciences South America Center for Astronomy, China-Chile Joint Center for Astronomy, Camino El Observatorio 1515, Las Condes, Santiago, Chile
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