C
C. Moni Bidin
Researcher at Catholic University of the North
Publications - 28
Citations - 1321
C. Moni Bidin is an academic researcher from Catholic University of the North. The author has contributed to research in topics: Globular cluster & Stars. The author has an hindex of 12, co-authored 28 publications receiving 1068 citations.
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Journal ArticleDOI
Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis
Maria R. Drout,Anthony L. Piro,Benjamin J. Shappee,Charles D. Kilpatrick,J. D. Simon,Carlos Contreras,David A. Coulter,R. J. Foley,Matthew R. Siebert,Nidia Morrell,Konstantina Boutsia,F. Di Mille,Thomas W.-S. Holoien,Daniel Kasen,Daniel Kasen,Juna A. Kollmeier,Barry F. Madore,Andrew J. Monson,Andrew J. Monson,Ariadna Murguia-Berthier,Yen-Chen Pan,Jason X. Prochaska,Enrico Ramirez-Ruiz,Enrico Ramirez-Ruiz,A. Rest,A. Rest,C. Adams,Katherine Alatalo,Katherine Alatalo,Eduardo Bañados,J. Baughman,J. Baughman,Timothy C. Beers,Timothy C. Beers,R. A. Bernstein,Theodoros Bitsakis,Abdo Campillay,Terese T. Hansen,C. R. Higgs,C. R. Higgs,Alexander P. Ji,Grigoris Maravelias,Jennifer L. Marshall,C. Moni Bidin,J. L. Prieto,J. L. Prieto,Kaitlin C. Rasmussen,Kaitlin C. Rasmussen,César Rojas-Bravo,A. L. Strom,N. Ulloa,J. Vargas-González,Z. Wan,Devin D. Whitten,Devin D. Whitten +54 more
TL;DR: In this paper, the authors present ultraviolet, optical, and infrared light curves of SSS17a extending from 10.9 hours to 18 days post-merger, showing that the late-time light curve indicates that SSS 17a produced at least 0.05 solar masses of heavy elements, demonstrating that neutron star mergers play a role in rapid neutron capture (r-process) nucleosynthesis in the universe.
Journal ArticleDOI
Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis
Maria R. Drout,Anthony L. Piro,Benjamin J. Shappee,Charles D. Kilpatrick,J. D. Simon,Carlos Contreras,David A. Coulter,R. J. Foley,Matthew R. Siebert,Nidia Morrell,Konstantina Boutsia,F. Di Mille,Thomas W.-S. Holoien,Daniel Kasen,Daniel Kasen,Juna A. Kollmeier,Barry F. Madore,Andrew J. Monson,Andrew J. Monson,Ariadna Murguia-Berthier,Yen-Chen Pan,Jason X. Prochaska,Enrico Ramirez-Ruiz,Enrico Ramirez-Ruiz,A. Rest,A. Rest,C. Adams,Katherine Alatalo,Katherine Alatalo,Eduardo Bañados,J. Baughman,J. Baughman,Timothy C. Beers,Timothy C. Beers,R. A. Bernstein,Theodoros Bitsakis,Abdo Campillay,Terese T. Hansen,C. R. Higgs,C. R. Higgs,Alexander P. Ji,Grigoris Maravelias,Jennifer L. Marshall,C. Moni Bidin,J. L. Prieto,J. L. Prieto,Kaitlin C. Rasmussen,Kaitlin C. Rasmussen,César Rojas-Bravo,A. L. Strom,N. Ulloa,J. Vargas-González,Z. Wan,Devin D. Whitten,Devin D. Whitten +54 more
TL;DR: The late-time light curve indicates that SSS17a produced at least ~0.05 solar masses of heavy elements, demonstrating that neutron star mergers play a role in rapid neutron capture (r-process) nucleosynthesis in the universe.
Journal ArticleDOI
A spectroscopic study of the globular cluster M28 (NGC 6626)
TL;DR: In this article, the abundance analysis for a sample of 17 red giant branch stars in the metal-poor globular cluster M28 based on high-resolution spectra was presented, and the authors derived abundances of O, Na, Mg, Al, Si, Ca, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, Y, Zr, Ba, La, Ce, and Eu.
Journal ArticleDOI
Chemical abundances of giant stars in NGC 5053 and NGC 5634, two globular clusters associated with the Sagittarius dwarf spheroidal galaxy?
Luca Sbordone,Luca Sbordone,Lorenzo Monaco,C. Moni Bidin,Piercarlo Bonifacio,S. Villanova,Michele Bellazzini,Rodrigo A. Ibata,Masashi Chiba,Douglas Geisler,Elisabetta Caffau,S. Duffau,S. Duffau +12 more
TL;DR: In this article, the authors analyze high-resolution and signal-to-noise spectra by means of the MyGIsFOS code, determining atmospheric parameters and abundances for up to 21 species between O and Eu.
Journal ArticleDOI
A spectroscopic study of the globular Cluster NGC 4147
TL;DR: In this paper, the abundance analysis for a sample of 18 red giant branch stars in the metal-poor globular cluster NGC 4147 based on medium and high resolution spectra is presented.