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Results 1 - 20 of 538  for All Library Resources

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1
Multi-epoch sampling of the radio star population with the Australian SKA Pathfinder
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Multi-epoch sampling of the radio star population with the Australian SKA Pathfinder

arXiv.org, 2023-12

2023. 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.2312.11031

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2
The influence of host star activity evolution on the population of super-Earths and mini-Neptunes
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The influence of host star activity evolution on the population of super-Earths and mini-Neptunes

arXiv.org, 2022-09

2022. 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.2209.05860

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3
The stochastic enrichment of Population II stars
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The stochastic enrichment of Population II stars

arXiv.org, 2020-10

2020. 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.2010.10532

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4
Rapid stellar and binary population synthesis with COMPAS
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Rapid stellar and binary population synthesis with COMPAS

arXiv.org, 2021-12

2021. 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.2109.10352

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5
Gravitational Microlensing Event Statistics for the Zwicky Transient Facility
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Gravitational Microlensing Event Statistics for the Zwicky Transient Facility

arXiv.org, 2020-06

2020. 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.2006.05439

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6
Fragmentation induced starvation in Population III star formation: a resolution study
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Fragmentation induced starvation in Population III star formation: a resolution study

arXiv.org, 2021-12

2021. 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.2112.10800

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7
The New Generation Planetary Population Synthesis (NGPPS). II. Planetary population of solar-like stars and overview of statistical results
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The New Generation Planetary Population Synthesis (NGPPS). II. Planetary population of solar-like stars and overview of statistical results

arXiv.org, 2021-10

2021. 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.2007.05562

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8
Tracing the Origins of Mass Segregation in M35: Evidence for Primordially Segregated Binaries
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Tracing the Origins of Mass Segregation in M35: Evidence for Primordially Segregated Binaries

arXiv.org, 2023-08

2023. 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.2308.13520

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9
When the Stars Align: A 5 {\sigma} Concordance of Planetary Nebulae Major Axes in the Centre of our Galaxy
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When the Stars Align: A 5 {\sigma} Concordance of Planetary Nebulae Major Axes in the Centre of our Galaxy

arXiv.org, 2023-07

2023. 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.2307.07140

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10
Chemically Homogeneous Evolution: A rapid population synthesis approach
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Chemically Homogeneous Evolution: A rapid population synthesis approach

arXiv.org, 2021-05

2021. 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.2010.00002

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11
Searching for Low-mass Population III Stars Disguised as White Dwarfs
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Searching for Low-mass Population III Stars Disguised as White Dwarfs

arXiv.org, 2021-02

2021. 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.2102.05058

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12
Following the Cosmic Evolution of Pristine Gas III: The Observational Consequences of the Unknown Properties of Population III Stars
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Following the Cosmic Evolution of Pristine Gas III: The Observational Consequences of the Unknown Properties of Population III Stars

arXiv.org, 2019-01

2019. 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.1901.03727

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13
Age dissection of the Milky Way discs: red giants in the Kepler field
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Age dissection of the Milky Way discs: red giants in the Kepler field

arXiv.org, 2020-11

2020. 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.2004.14806

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14
Benchmarking Gaia DR3 Apsis with the Hyades and Pleiades open clusters
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Benchmarking Gaia DR3 Apsis with the Hyades and Pleiades open clusters

arXiv.org, 2023-08

2023. 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.2306.03132

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15
Observed binary populations reflect the Galactic history. Explaining the orbital period-mass ratio relation in wide hot subdwarf binaries
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Observed binary populations reflect the Galactic history. Explaining the orbital period-mass ratio relation in wide hot subdwarf binaries

arXiv.org, 2020-08

2020. 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.2003.05665

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16
Wide binaries are rare in open clusters
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Wide binaries are rare in open clusters

arXiv.org, 2020-06

2020. 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.2006.06679

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17
Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe
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Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe

arXiv.org, 2022-03

2022. 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.2112.07469

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18
The Local Group Symbiotic Star Population and its Weak Relation with Type Ia Supernovae
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The Local Group Symbiotic Star Population and its Weak Relation with Type Ia Supernovae

arXiv.org, 2023-09

2023. 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.2309.04466

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19
First Light II: Emission Line Extinction, Population III Stars, and X-ray Binaries
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First Light II: Emission Line Extinction, Population III Stars, and X-ray Binaries

arXiv.org, 2017-12

2017. 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.1709.04473

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20
Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS
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Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS

arXiv.org, 2022-10

2022. 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.2206.13842

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