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1 |
Material Type: Article
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Multi-epoch sampling of the radio star population with the Australian SKA PathfinderarXiv.org, 2023-122023. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://creativecommons.org/licenses/by/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2312.11031Full text available |
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2 |
Material Type: Article
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The influence of host star activity evolution on the population of super-Earths and mini-NeptunesarXiv.org, 2022-092022. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2209.05860Full text available |
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3 |
Material Type: Article
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The stochastic enrichment of Population II starsarXiv.org, 2020-102020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2010.10532Full text available |
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4 |
Material Type: Article
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Rapid stellar and binary population synthesis with COMPASarXiv.org, 2021-122021. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2109.10352Full text available |
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5 |
Material Type: Article
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Gravitational Microlensing Event Statistics for the Zwicky Transient FacilityarXiv.org, 2020-062020. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://creativecommons.org/licenses/by/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2006.05439Full text available |
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6 |
Material Type: Article
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Fragmentation induced starvation in Population III star formation: a resolution studyarXiv.org, 2021-122021. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2112.10800Full text available |
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7 |
Material Type: Article
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The New Generation Planetary Population Synthesis (NGPPS). II. Planetary population of solar-like stars and overview of statistical resultsarXiv.org, 2021-102021. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2007.05562Full text available |
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8 |
Material Type: Article
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Tracing the Origins of Mass Segregation in M35: Evidence for Primordially Segregated BinariesarXiv.org, 2023-082023. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2308.13520Full text available |
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9 |
Material Type: Article
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When the Stars Align: A 5 {\sigma} Concordance of Planetary Nebulae Major Axes in the Centre of our GalaxyarXiv.org, 2023-072023. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://creativecommons.org/licenses/by/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2307.07140Full text available |
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10 |
Material Type: Article
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Chemically Homogeneous Evolution: A rapid population synthesis approacharXiv.org, 2021-052021. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2010.00002Full text available |
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11 |
Material Type: Article
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Searching for Low-mass Population III Stars Disguised as White DwarfsarXiv.org, 2021-022021. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2102.05058Full text available |
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12 |
Material Type: Article
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Following the Cosmic Evolution of Pristine Gas III: The Observational Consequences of the Unknown Properties of Population III StarsarXiv.org, 2019-012019. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1901.03727Full text available |
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13 |
Material Type: Article
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Age dissection of the Milky Way discs: red giants in the Kepler fieldarXiv.org, 2020-112020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2004.14806Full text available |
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14 |
Material Type: Article
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Benchmarking Gaia DR3 Apsis with the Hyades and Pleiades open clustersarXiv.org, 2023-082023. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://creativecommons.org/licenses/by/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2306.03132Full text available |
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15 |
Material Type: Article
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Observed binary populations reflect the Galactic history. Explaining the orbital period-mass ratio relation in wide hot subdwarf binariesarXiv.org, 2020-082020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2003.05665Full text available |
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16 |
Material Type: Article
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Wide binaries are rare in open clustersarXiv.org, 2020-062020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2006.06679Full text available |
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17 |
Material Type: Article
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Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNearXiv.org, 2022-032022. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2112.07469Full text available |
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18 |
Material Type: Article
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The Local Group Symbiotic Star Population and its Weak Relation with Type Ia SupernovaearXiv.org, 2023-092023. This work is published under http://creativecommons.org/licenses/by-nc-sa/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://creativecommons.org/licenses/by-nc-sa/4.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2309.04466Full text available |
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19 |
Material Type: Article
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First Light II: Emission Line Extinction, Population III Stars, and X-ray BinariesarXiv.org, 2017-122017. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1709.04473Full text available |
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20 |
Material Type: Article
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Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASSarXiv.org, 2022-102022. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2206.13842Full text available |