1,721,004 research outputs found
Stellar Populations as Building Blocks of Galaxies (IAU S241)
No full textPreface; 1. Model ingredients: stellar evolution models; 2. Model ingredients: stellar spectral libraries; 3. Initial mass function; 4. Stellar population models; 5. Stellar populations in the Milky Way; 6. Resolved stellar populations in the Local Group; 7. Stellar populations in early-type galaxies; 8. Extragalactic globular cluster systems; 9. Stellar populations in late-type galaxies; 10. Stellar populations at higher redshifts; 11. New observing facilities; Author index
Stellar Populations as Building Blocks of Galaxies (IAU S241)
No full textPreface; 1. Model ingredients: stellar evolution models; 2. Model ingredients: stellar spectral libraries; 3. Initial mass function; 4. Stellar population models; 5. Stellar populations in the Milky Way; 6. Resolved stellar populations in the Local Group; 7. Stellar populations in early-type galaxies; 8. Extragalactic globular cluster systems; 9. Stellar populations in late-type galaxies; 10. Stellar populations at higher redshifts; 11. New observing facilities; Author index
Stellar Populations as Building Blocks of Galaxies (IAU S241)
No full textPreface; 1. Model ingredients: stellar evolution models; 2. Model ingredients: stellar spectral libraries; 3. Initial mass function; 4. Stellar population models; 5. Stellar populations in the Milky Way; 6. Resolved stellar populations in the Local Group; 7. Stellar populations in early-type galaxies; 8. Extragalactic globular cluster systems; 9. Stellar populations in late-type galaxies; 10. Stellar populations at higher redshifts; 11. New observing facilities; Author index
Stellar Populations as Building Blocks of Galaxies (IAU S241)
No full textPreface; 1. Model ingredients: stellar evolution models; 2. Model ingredients: stellar spectral libraries; 3. Initial mass function; 4. Stellar population models; 5. Stellar populations in the Milky Way; 6. Resolved stellar populations in the Local Group; 7. Stellar populations in early-type galaxies; 8. Extragalactic globular cluster systems; 9. Stellar populations in late-type galaxies; 10. Stellar populations at higher redshifts; 11. New observing facilities; Author index
Stellar Populations as Building Blocks of Galaxies (IAU S241)
No full textPreface; 1. Model ingredients: stellar evolution models; 2. Model ingredients: stellar spectral libraries; 3. Initial mass function; 4. Stellar population models; 5. Stellar populations in the Milky Way; 6. Resolved stellar populations in the Local Group; 7. Stellar populations in early-type galaxies; 8. Extragalactic globular cluster systems; 9. Stellar populations in late-type galaxies; 10. Stellar populations at higher redshifts; 11. New observing facilities; Author index
Stellar Populations as Building Blocks of Galaxies (IAU S241)
No full textPreface; 1. Model ingredients: stellar evolution models; 2. Model ingredients: stellar spectral libraries; 3. Initial mass function; 4. Stellar population models; 5. Stellar populations in the Milky Way; 6. Resolved stellar populations in the Local Group; 7. Stellar populations in early-type galaxies; 8. Extragalactic globular cluster systems; 9. Stellar populations in late-type galaxies; 10. Stellar populations at higher redshifts; 11. New observing facilities; Author index
Stellar Populations as Building Blocks of Galaxies (IAU S241)
No full textPreface; 1. Model ingredients: stellar evolution models; 2. Model ingredients: stellar spectral libraries; 3. Initial mass function; 4. Stellar population models; 5. Stellar populations in the Milky Way; 6. Resolved stellar populations in the Local Group; 7. Stellar populations in early-type galaxies; 8. Extragalactic globular cluster systems; 9. Stellar populations in late-type galaxies; 10. Stellar populations at higher redshifts; 11. New observing facilities; Author index
Stellar Populations as Building Blocks of Galaxies (IAU S241)
No full textPreface; 1. Model ingredients: stellar evolution models; 2. Model ingredients: stellar spectral libraries; 3. Initial mass function; 4. Stellar population models; 5. Stellar populations in the Milky Way; 6. Resolved stellar populations in the Local Group; 7. Stellar populations in early-type galaxies; 8. Extragalactic globular cluster systems; 9. Stellar populations in late-type galaxies; 10. Stellar populations at higher redshifts; 11. New observing facilities; Author index
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
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