DB
D. Belloni
astro-ph.SRastro-ph.GAastro-ph.HEastro-ph.EPastro-ph.IM
On Valency
published · living versionsW_r5msuqva·v1 · currentpublished
The evolutionary history of ultra-compact accreting binaries. II. HST spectroscopy of two eclipsing AM CVn stars
with W. Yu, A. F. Pala, T. Kupfer, B. T. Gänsicke +48
1 version
Preprints & journals
54 papers in the corpus · 2016–2026A Comprehensive Study of the Long-Period Cataclysmic Variable V630 Cassiopeiae2609.30669v1 · Ivan Mora Zamora, Gagik Tovmassian, Juan Echevarria et al.2026 · 0 citationsarXiv
Dynamical formation of long-period exoplanets systems in evolving binary stars2607.19118v1 · Isabel J. Lima, Rafael R. Sousa, Silvia M. Giuliatti Winter et al.2026 · 0 citationsarXiv
Influence of mass-transfer stability on the formation of post-common-envelope binaries2606.22927v2 · Yanxu Shi, Hongwei Ge, Zhenwei Li et al.2026 · 0 citationsarXiv
Evolution of a long-period Cataclysmic Variable from the viewpoint of the donor star: the case of SDSS J085210.48+783246.62605.24347v1 · G. Tovmassian, D. Belloni, I. Mora Zamora et al.2026 · 0 citationsarXiv
No Period Change in Two Long-Period AM CVn Binaries2604.06460v1 · Matthew J. Green, Thomas R. Marsh, Jan van Roestel et al.2026 · 0 citationsarXiv
A modest change in magnetic braking at the fully convective boundary explains cataclysmic variable evolution2603.14560v1 · Joaqu'in A. Barraza-Jorquera, Matthias R. Schreiber, Stuart Littlefair et al.2026 · 4 citationsA&A 708, L11 (2026)
Distance Estimation and Sky Localization of Eccentric Double White Dwarf Binaries from Gravitational Wave Observations inside Globular Clusters2602.10664v1 · Yuetong Zhao, L. Hellstrom, Siqi Zhang et al.2026 · 0 citationsarXiv
From Main Sequence Binary to Blast: MESA Modeling of the Double-Detonation Progenitor PTF1~J2238+74302602.04421v1 · Mercedes S. Hernandez, Thomas Kupfer, Diogo Belloni et al.2026 · 2 citationsarXiv
Predicted incidence of Jupiter-like planets around white dwarfs2601.19531v1 · Alex Mauch-Soriano, Matthias R. Schreiber, Diego Correa et al.2026 · 0 citationsarXiv
White Dwarfs in Wide Binary Systems as Reliable Age Calibrators2512.14769v1 · Alberto Rebassa-Mansergas, Roberto Raddi, Anna F. Pala et al.2025 · 0 citationsarXiv
Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagitarii2508.21358v2 · Gagik Tovmassian, Diogo Belloni, Anna F. Pala et al.2025 · 4 citationsA&A 703, A119 (2025)
The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields2505.24153v1 · Matthias R. Schreiber, Diogo Belloni2025 · 4 citationsarXiv
Further evidence of saturated, boosted, and disrupted magnetic braking from evolutionary tracks of cataclysmic variables2503.18884v2 · Joaqu'in A. Barraza-Jorquera, Matthias R. Schreiber, Diogo Belloni2025 · 13 citationsarXiv
Resolution of a paradox: SDSS J1257+5428 can be explained as a descendant of a cataclysmic variable with an evolved donor2503.16204v1 · Diogo Belloni, Matthias R. Schreiber, Kareem El-Badry2025 · 5 citationsarXiv
A second candidate magnetic helium core white dwarf and 3 other variable white dwarfs in the globular cluster NGC 63972412.12375v1 · Manuel Pichardo Marcano, Liliana E. Rivera Sandoval, Thomas J. Maccarone et al.2024 · 3 citationsarXiv
Suggested magnetic braking prescription derived from field complexity fails to reproduce the cataclysmic variable orbital period gap2409.05673v1 · Valentina Ort'uzar-Garz'on, Matthias R. Schreiber, Diogo Belloni2024 · 5 citationsarXiv
Double white dwarf binary population in MOCCA star clusters -- Comparisons with observations of close and wide binaries2405.04314v3 · Lucas Hellstrom, Miros\law Giersz, Arkadiusz Hypki et al.2024 · 1 citationA&A 690, A112 (2024)
Reevaluating the Origin of Detectable Cataclysmic Variables in Globular Clusters: Testing the Importance of Dynamics2404.03796v1 · Liliana Rivera Sandoval, Diogo Belloni, Miriam Ramos Arevalo2024 · 2 citationsThe Astrophysical Journal Letters, Volume 964, Number 2, 2024
The formation of the magnetic symbiotic star FN Sgr2402.08647v2 · Diogo Belloni, Joanna Miko\lajewska, Matthias R. Schreiber2024 · 12 citationsA&A 686, A226 (2024)
The cataclysmic variable orbital period gap: More evident than ever2402.02076v1 · Matthias R. Schreiber, Diogo Belloni, Axel D. Schwope2024 · 37 citationsarXiv
Formation of long-period post-common-envelope binaries II. Explaining the self-lensing binary KOI 32782401.17510v2 · Diogo Belloni, Matthias R. Schreiber, Monica Zorotovic2024 · 17 citationsA&A 687, A12 (2024)
Formation of long-period post-common-envelope binaries I. No extra energy is needed to explain oxygen-neon white dwarfs paired with AFGK-type main-sequence stars2401.07692v2 · Diogo Belloni, Monica Zorotovic, Matthias R. Schreiber et al.2024 · 20 citationsA&A 686, A61 (2024)
A Chandra Survey of Milky Way Globular Clusters -- IV. Periodic X-ray sources2311.14511v1 · Tong Bao, Zhiyuan Li, Zhongqun Cheng et al.2023 · 7 citationsarXiv
Evidence for saturated and disrupted magnetic braking from samples of detached close binaries with M and K dwarfs2311.04309v1 · Diogo Belloni, Matthias R. Schreiber, Maxwell Moe et al.2023 · 23 citationsarXiv
Period bouncers as detached magnetic cataclysmic variables2310.17276v1 · Matthias R. Schreiber, Diogo Belloni, Jan van Roestel2023 · 25 citationsarXiv
Reversing the verdict: Cataclysmic variables could be the dominant progenitors of AM CVn binaries after all2305.19312v2 · Diogo Belloni, Matthias R. Schreiber2023 · 29 citationsA&A 678, A34 (2023)
Formation and Evolution of Accreting Compact Objects2303.08997v3 · Diogo Belloni, Matthias R. Schreiber2023 · 19 citationsarXiv
A candidate magnetic helium core white dwarf in the globular cluster NGC 63972303.04184v1 · Manuel Pichardo Marcano, Liliana E. Rivera Sandoval, Thomas J. Maccarone et al.2023 · 4 citationsarXiv
MOCCA: Dynamics and evolution of binary stars of multiple stellar populations in tidally filling and underfilling globular star clusters2205.05397v2 · Arkadiusz Hypki, Mirek Giersz, Jongsuk Hong et al.2022 · 27 citationsarXiv
Magnetic dynamos in white dwarfs -III: explaining the occurrence of strong magnetic fields in close double white dwarfs2204.07901v1 · Matthias.R. Schreiber, Diogo Belloni, Monica Zorotovic et al.2022 · 25 citationsarXiv
The White Dwarf Binary Pathways Survey VII: Evidence for a bi-modal distribution of post mass transfer systems?2203.08846v1 · F. Lagos, M. R. Schreiber, S.G. Parsons et al.2022 · 20 citationsarXiv
Constraining the Evolution of Cataclysmic Variables via the Masses and Accretion Rates of their Underlying White Dwarfs2111.13706v1 · A. F. Pala, B. T. Gansicke, D. Belloni et al.2021 · 119 citationsarXiv
Breaking the degeneracy in magnetic cataclysmic variable X-ray spectral modeling using X-ray light curves2107.10861v1 · Diogo Belloni, Claudia V. Rodrigues, Matthias R. Schreiber et al.2021 · 9 citationsarXiv
Magnetic dynamos in white dwarfs -- II. Relating magnetism and pollution2106.09727v1 · Matthias R. Schreiber, Diogo Belloni, Boris T. Gaensicke et al.2021 · 20 citationsarXiv
Magnetic dynamos in white dwarfs -- I. Explaining the dearth of bright intermediate polars in globular clusters2105.11459v1 · Diogo Belloni, Matthias R. Schreiber, Maurizio Salaris et al.2021 · 18 citationsarXiv
Preparing the next gravitational million-body simulations: Evolution of single and binary stars in Nbody6++GPU, MOCCA and McLuster2105.08067v2 · A. W. H. Kamlah, A. Leveque, R. Spurzem et al.2021 · 74 citationsarXiv
The origin and evolution of magnetic white dwarfs in close binary stars2104.14607v1 · Matthias R. Schreiber, Diogo Belloni, Boris T. Gaensicke et al.2021 · 126 citationsPublished by Nature Astronomy (2021)
Search for magnetic accretion in SW Sextantis systems2103.02007v1 · I. J. Lima, C. V. Rodrigues, C. E. Ferreira Lopes et al.2021 · 7 citationsarXiv
Properties of Cataclysmic Variables in Globular Clusters2008.12772v1 · Diogo Belloni, Liliana E. Rivera Sandoval2020 · 12 citationsarXiv
On the absence of symbiotic stars in globular clusters2004.05453v2 · Diogo Belloni, Joanna Miko\lajewska, Krystian I\lkiewicz et al.2020 · 19 citationsarXiv
Are white dwarf magnetic fields in close binaries generated during common-envelope evolution?1910.08582v2 · Diogo Belloni, Matthias R. Schreiber2019 · 24 citationsarXiv
Evidence for reduced magnetic braking in polars from binary population models1910.06333v2 · Diogo Belloni, Matthias R. Schreiber, Anna F. Pala et al.2019 · 78 citationsarXiv
Optical observations and cyclops post-shock region modelling of the polar V348 Pav1909.00874v1 · Alexandre S. Oliveira, Claudia V. Rodrigues, Matheus S. Palhares et al.2019 · 6 citationsarXiv
Are most Cataclysmic Variables in Globular Clusters dynamically formed?1907.06527v1 · Diogo Belloni, Mirek Giersz, Liliana E. Rivera Sandoval et al.2019 · 1 citationarXiv
MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- IV. cataclysmic variables -- properties of bright and faint populations1811.04937v1 · Diogo Belloni, Mirek Giersz, Liliana E. Rivera Sandoval et al.2018 · 55 citationsarXiv
No cataclysmic variables missing: higher merger rate brings into agreement observed and predicted space densities1806.05687v1 · Diogo Belloni, Matthias R. Schreiber, M'onica Zorotovic et al.2018 · 55 citationsarXiv
The origin of the first neutron star -- neutron star merger1712.00632v3 · K. Belczynski, A. Askar, M. Arca-Sedda et al.2017 · 120 citationsarXiv
Dynamical equivalence, the origin of the Galactic field stellar and binary population, and the initial radius--mass relation of embedded clusters1711.07987v2 · Diogo Belloni, Pavel Kroupa, Helio J. Rocha-Pinto et al.2017 · 20 citationsarXiv
On the initial binary population for star cluster simulations1707.04271v1 · Diogo Belloni, Abbas Askar, Mirek Giersz et al.2017 · 67 citationsarXiv
MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- III. Cataclysmic variables -- Implications of model assumptions1703.01838v1 · Diogo Belloni, M'onica Zorotovic, Matthias R. Schreiber et al.2017 · 23 citationsarXiv
Career total: 85 works. 54 are in this corpus.Showing the 50 most recent.
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