( en | de | ru )

 

Disambiguation

From post

копироватьудалитьдобавить публикацию в буфер
The Stellar Initial Mass Function in Early-Type Galaxies From Absorption Line Spectroscopy. IV. A Super-Salpeter IMF in the center of NGC 1407 from Non-Parametric Models

, , и . (2016)cite arxiv:1612.00013Comment: 7 pages, 6 figures, submitted to ApJ.

Please choose a person to relate this publication to

To differ between persons with the same name, the academic degree and the title of an important publication will be displayed.

Charlie Przetak

Charlie Hargood

Charlie Mahn

Charlie Mansfield

Charlie al- Farr

 

Другие публикации лиц с тем же именем

Future Prospects: Deep Imaging of Galaxy Outskirts using Telescopes Large and Small, , , , , , , и . (2016)cite arxiv:1612.06415Comment: 27 pages, 10 figures, Invited review, Book chapter in Öutskirts of Galaxies", Eds. J. H. Knapen, J. C. Lee and A. Gil de Paz, Astrophysics and Space Science Library, Springer, in press.A High Stellar Velocity Dispersion and ~100 Globular Clusters for the Ultra Diffuse Galaxy Dragonfly 44, , , , , , , , и . (2016)cite arxiv:1606.06291Comment: Submitted to ApJ Letters.Nebular Continuum and Line Emission in Stellar Population Synthesis Models, , , и . (2016)cite arxiv:1611.08305Comment: 35 pages, 29 figures.Signatures of unresolved binaries in stellar spectra: implications for spectral fitting, , , , , , , и . (2017)cite arxiv:1709.03983Comment: Submitted to MNRAS. 7 pages, 5 figures.Forty-Seven Milky Way-Sized, Extremely Diffuse Galaxies in the Coma Cluster, , , , , и . (2014)cite arxiv:1410.8141Comment: Submitted to ApJ Letters. To illustrate how big and fluffy these things are we made a graphic comparing the one with ACS imaging (Fig 4) to several well-known galaxies, if they were at the same distance: http://www.astro.yale.edu/dokkum/coma_udgs/sizes.jpg.The SINFONI Nearby Elliptical Lens Locator Survey: Discovery of two new low-redshift strong lenses and implications for the initial mass function in giant early-type galaxies, , и . (2015)cite arxiv:1503.02661Comment: Accepted for publication in MNRAS.Pixel Color Magnitude Diagrams for Semi-Resolved Stellar Populations: The Star Formation History of Regions within the Disk and Bulge of M31, и . (2016)cite arxiv:1602.05580Comment: 11 pages, 9 figures, submitted to ApJ.Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?, , , , , , , , , и 15 other автор(ы). (2022)cite arxiv:2208.02794Comment: Submitted to ApJL. Fig. 1 shows the "superposed" state, Fig. 2 presents the potential z~5 protocluster, Fig. 3 shows some atypical z~5 SEDs, Fig. 4 studies the morphology, Fig. 5 summarizes the extraordinary situation at z~17, and Fig. 6 argues for why such interlopers may not be a major issue for z>10 searches. Comments warmly welcomed.The Stellar Initial Mass Function in Early-Type Galaxies From Absorption Line Spectroscopy. I. Data and Empirical Trends, и . (2012)cite arxiv:1205.6471Comment: Submitted to the Astrophysical Journal. 14 pages, 12 figures. With an Appendix re-examining van Dokkum (2008).The stellar IMF determined in early-type galaxies from a non-degenerate set of optical line indices, , , и . (2013)cite arxiv:1305.2873Comment: 15 pages, 9 figures.