Results 1 - 20 of 52,040 for All Library Resources
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| Result Number | Material Type | Add to My Shelf Action | Record Details and Options |
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| 1 |
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A triple protostar system formed via fragmentation of a gravitationally unstable diskNature (London), 2016-10, Vol.538 (7626), p.483-486 [Peer Reviewed Journal]COPYRIGHT 2016 Nature Publishing Group ;COPYRIGHT 2016 Nature Publishing Group ;Copyright Nature Publishing Group Oct 27, 2016 ;ISSN: 0028-0836 ;ISSN: 1476-4687 ;EISSN: 1476-4687 ;DOI: 10.1038/nature20094 ;PMID: 27786204 ;CODEN: NATUASFull text available |
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The REQUIEM Survey. I. A Search for Extended Lyα Nebular Emission Around 31 z > 5.7 QuasarsThe Astrophysical journal, 2019-12, Vol.887 (2), p.196 [Peer Reviewed Journal]Copyright IOP Publishing Dec 20, 2019 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab5847Full text available |
| 3 |
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Properties of galaxies reproduced by a hydrodynamic simulationNature (London), 2014-05, Vol.509 (7499), p.177-182 [Peer Reviewed Journal]COPYRIGHT 2014 Nature Publishing Group ;COPYRIGHT 2014 Nature Publishing Group ;Copyright Nature Publishing Group May 8, 2014 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/nature13316 ;PMID: 24805343 ;CODEN: NATUASFull text available |
| 4 |
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New Determinations of the UV Luminosity Functions from z ∼ 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation EfficiencyThe Astronomical journal, 2021-08, Vol.162 (2), p.47 [Peer Reviewed Journal]2021. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Aug 2021 ;ISSN: 0004-6256 ;ISSN: 1538-3881 ;EISSN: 1538-3881 ;DOI: 10.3847/1538-3881/abf83eFull text available |
| 5 |
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Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emissionNature (London), 2015-06, Vol.522 (7557), p.455-458 [Peer Reviewed Journal]Copyright Nature Publishing Group Jun 25, 2015 ;Attribution ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/nature14500 ;PMID: 26108853 ;CODEN: NATUASFull text available |
| 6 |
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Identification and properties of intense star-forming galaxies at redshifts z > 10Nature astronomy, 2023-05, Vol.7 (5), p.611-621 [Peer Reviewed Journal]Distributed under a Creative Commons Attribution 4.0 International License ;EISSN: 2397-3366 ;DOI: 10.1038/s41550-023-01921-1Full text available |
| 7 |
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The host galaxy of a fast radio burstNature (London), 2016-02, Vol.530 (7591), p.453-456 [Peer Reviewed Journal]COPYRIGHT 2016 Nature Publishing Group ;COPYRIGHT 2016 Nature Publishing Group ;Copyright Nature Publishing Group Feb 25, 2016 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/nature17140 ;PMID: 26911781 ;CODEN: NATUASFull text available |
| 8 |
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The first gravitational-wave source from the isolated evolution of two stars in the 40-100 solar mass rangeNature (London), 2016-06, Vol.534 (7608), p.512-515 [Peer Reviewed Journal]COPYRIGHT 2016 Nature Publishing Group ;COPYRIGHT 2016 Nature Publishing Group ;Copyright Nature Publishing Group Jun 23, 2016 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/nature18322 ;PMID: 27337338 ;CODEN: NATUASFull text available |
| 9 |
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Quiescent Galaxies 1.5 Billion Years after the Big Bang and Their ProgenitorsThe Astrophysical journal, 2020-02, Vol.889 (2), p.93 [Peer Reviewed Journal]2020. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Feb 01, 2020 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab64dcFull text available |
| 10 |
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Disk-mediated accretion burst in a high-mass young stellar objectNature physics, 2017-03, Vol.13 (3), p.276-279 [Peer Reviewed Journal]Copyright Nature Publishing Group Mar 2017 ;ISSN: 1745-2473 ;EISSN: 1745-2481 ;DOI: 10.1038/nphys3942Full text available |
| 11 |
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A unified multiwavelength model of galaxy formationMonthly notices of the Royal Astronomical Society, 2016-11, Vol.462, p.3854-3911 [Peer Reviewed Journal]Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1093/mnras/stw1888Digital Resources/Online E-Resources |
| 12 |
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When Do Stalled Stars Resume Spinning Down? Advancing Gyrochronology with Ruprecht 147The Astrophysical journal, 2020-12, Vol.904 (2), p.140 [Peer Reviewed Journal]2020. The Author(s). Published by the American Astronomical Society. ;Copyright IOP Publishing Dec 01, 2020 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/abbf58Full text available |
| 13 |
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The merger that led to the formation of the Milky Way's inner stellar halo and thick diskNature (London), 2018-11, Vol.563 (7729), p.85-88 [Peer Reviewed Journal]COPYRIGHT 2018 Nature Publishing Group ;COPYRIGHT 2018 Nature Publishing Group ;Copyright Nature Publishing Group Nov 1, 2018 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/s41586-018-0625-x ;PMID: 30382207Full text available |
| 14 |
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The Recent Burstiness of Star Formation in Galaxies at z ∼ 4.5 from Hα MeasurementsThe Astrophysical journal, 2019-10, Vol.884 (2), p.133 [Peer Reviewed Journal]Copyright IOP Publishing Oct 20, 2019 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab425bFull text available |
| 15 |
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CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWSTAstrophysical journal. Letters, 2023-03, Vol.946 (1), p.L13 [Peer Reviewed Journal]2023. The Author(s). Published by the American Astronomical Society. ;2023. The Author(s). Published by the American Astronomical Society. 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. ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 2041-8205 ;EISSN: 2041-8213 ;DOI: 10.3847/2041-8213/acade4Full text available |
| 16 |
Material Type: Article
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An ultraluminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30Nature (London), 2015-02, Vol.518 (7540), p.512-515 [Peer Reviewed Journal]COPYRIGHT 2015 Nature Publishing Group ;COPYRIGHT 2015 Nature Publishing Group ;Copyright Nature Publishing Group Feb 26, 2015 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/nature14241 ;PMID: 25719667 ;CODEN: NATUASFull text available |
| 17 |
Material Type: Article
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The formation of submillimetre-bright galaxies from gas infall over a billion yearsNature (London), 2015-09, Vol.525 (7570), p.496-499 [Peer Reviewed Journal]Copyright Nature Publishing Group Sep 24, 2015 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/nature15383 ;PMID: 26399829 ;CODEN: NATUASFull text available |
| 18 |
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A kilonova following a long-duration gamma-ray burst at 350 MpcNature (London), 2022-12, Vol.612 (7939), p.223-8 [Peer Reviewed Journal]2022. The Author(s), under exclusive licence to Springer Nature Limited. ;Copyright Nature Publishing Group Dec 8, 2022 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/s41586-022-05390-w ;PMID: 36477128Full text available |
| 19 |
Material Type: Article
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Star formation near the Sun is driven by expansion of the Local BubbleNature (London), 2022-01, Vol.601 (7893), p.334-337 [Peer Reviewed Journal]2022. The Author(s), under exclusive licence to Springer Nature Limited. ;Copyright Nature Publishing Group Jan 20, 2022 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/s41586-021-04286-5 ;PMID: 35022612Full text available |
| 20 |
Material Type: Article
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Regulation of star formation in giant galaxies by precipitation, feedback and conductionNature (London), 2015-03, Vol.519 (7542), p.203-206 [Peer Reviewed Journal]COPYRIGHT 2015 Nature Publishing Group ;COPYRIGHT 2015 Nature Publishing Group ;Copyright Nature Publishing Group Mar 12, 2015 ;ISSN: 0028-0836 ;EISSN: 1476-4687 ;DOI: 10.1038/nature14167 ;PMID: 25739501 ;CODEN: NATUASFull text available |
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