Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
New models for the evolution of post-asymptotic giant branch stars and central stars of planetary nebulae
2016262 citationsM. M. Miller BertolamiAmericanae (AECID Library)profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
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Countries citing papers authored by M. M. Miller Bertolami
Since
Specialization
Citations
This map shows the geographic impact of M. M. Miller Bertolami's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by M. M. Miller Bertolami with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. M. Miller Bertolami more than expected).
Fields of papers citing papers by M. M. Miller Bertolami
This network shows the impact of papers produced by M. M. Miller Bertolami. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by M. M. Miller Bertolami. The network helps show where M. M. Miller Bertolami may publish in the future.
Co-authorship network of co-authors of M. M. Miller Bertolami
This figure shows the co-authorship network connecting the top 25 collaborators of M. M. Miller Bertolami.
A scholar is included among the top collaborators of M. M. Miller Bertolami based on the total number of
citations received by their joint publications. Widths of edges
represent the number of papers authors have co-authored together.
Node borders
signify the number of papers an author published with M. M. Miller Bertolami. M. M. Miller Bertolami is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Ronco, María Paula, M. R. Schreiber, E. Villaver, O. M. Guilera, & M. M. Miller Bertolami. (2023). Planet formation around intermediate-mass stars. Astronomy and Astrophysics. 682. A155–A155.6 indexed citations
Bertolami, M. M. Miller, et al.. (2019). Asteroseismic signatures of the helium core flash. El Servicio de Difusión de la Creación Intelectual (National University of La Plata).10 indexed citations
Bertolami, M. M. Miller, et al.. (2019). Hunting young white dwarfs at the Center of Planetary Nebulae. Conicet.3 indexed citations
11.
Camisassa, María E., L. G. Althaus, A. H. Córsico, et al.. (2019). The evolution of ultra-massive white dwarfs. Springer Link (Chiba Institute of Technology).89 indexed citations
Camisassa, María E., L. G. Althaus, A. H. Córsico, et al.. (2016). The effect of <SUP>22</SUP>Ne diffusion in the evolution and pulsational properties of white dwarfs with solar metallicity progenitors. El Servicio de Difusión de la Creación Intelectual (National University of La Plata).52 indexed citations
14.
Bertolami, M. M. Miller. (2016). New models for the evolution of post-asymptotic giant branch stars and central stars of planetary nebulae. Americanae (AECID Library).262 indexed citations breakdown →
15.
Bertolami, M. M. Miller, et al.. (2014). Revisiting the axion bounds from the Galactic white dwarf luminosity function. El Servicio de Difusión de la Creación Intelectual (National University of La Plata).123 indexed citations
16.
Bertolami, M. M. Miller, et al.. (2013). Pulsations driven by the ε-mechanism in post-merger remnants: First results. El Servicio de Difusión de la Creación Intelectual (National University of La Plata).2 indexed citations
17.
Bertolami, M. M. Miller, L. G. Althaus, & E. Garcı́a–Berro. (2013). Quiescent nuclear burning in low-metallicity white dwarfs. El Servicio de Difusión de la Creación Intelectual (National University of La Plata).18 indexed citations
18.
Bertolami, M. M. Miller, et al.. (2011). On the challenging variability of LS IV-14°116: Pulsational instabilities excited by the ε-mechanism. El Servicio de Difusión de la Creación Intelectual (National University of La Plata).19 indexed citations
Bertolami, M. M. Miller, et al.. (2005). The formation of DA white dwarfs with thin Hydrogen envelopes through a late thermal pulse. 48. 185–191.2 indexed citations
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive
bibliographic database. While OpenAlex provides broad and valuable coverage of the global
research landscape, it—like all bibliographic datasets—has inherent limitations. These include
incomplete records, variations in author disambiguation, differences in journal indexing, and
delays in data updates. As a result, some metrics and network relationships displayed in
Rankless may not fully capture the entirety of a scholar's output or impact.