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1	$PDRs4All VII. The 3.3 $\mu$m aromatic infrared band as a tracer of physical properties of the ISM in galaxies$ $PDRs4All VII. The 3.3 $\mu$m aromatic infrared band as a tracer of physical properties of the ISM in galaxies$ Material Type: Article	PDRs4All VII. The 3.3 $\mu$m aromatic infrared band as a tracer of physical properties of the ISM in galaxies http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2402.16535 Digital Resources/Online E-Resources View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
2	Material Type: Article	Time variability of ultra-fast BAL outflows using SALT: C IV absorption depth based analysis Monthly notices of the Royal Astronomical Society. Letters, 2024-01, Vol.527 (4), p.12298-12309 http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 1745-3933 ;EISSN: 1745-3933 ;DOI: 10.48550/arxiv.2312.17320 Digital Resources/Online E-Resources View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
3	Material Type: Article	PDRs4All VI: Probing the Photochemical Evolution of PAHs in the Orion Bar Using Machine Learning Techniques Astronomy and astrophysics (Berlin), 2023-11, Vol.685 [Peer Reviewed Journal] 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 ;Attribution ;ISSN: 0004-6361 ;EISSN: 2331-8422 ;EISSN: 1432-0746 ;DOI: 10.48550/arxiv.2311.01163 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
4	Material Type: Article	PDRs4All. V. Modelling the dust evolution across the illuminated edge of the Orion Bar arXiv.org, 2024-01 [Peer Reviewed Journal] 2024. 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.2401.01221 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
5	Material Type: Article	ALMA-IMF IX: Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters The Astrophysical journal, 2023-10 [Peer Reviewed Journal] 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 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-637X ;EISSN: 2331-8422 ;EISSN: 1538-4357 ;DOI: 10.48550/arxiv.2310.13125 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
6	Material Type: Article	GOODS-ALMA 2.0: Last gigayear star formation histories of the so-called starbursts within the main sequence Astronomy and astrophysics (Berlin), 2022-11 [Peer Reviewed Journal] 2022. 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 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 2331-8422 ;EISSN: 1432-0746 ;DOI: 10.48550/arxiv.2211.02510 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
7	Material Type: Article	PDRs4All III: JWST's NIR spectroscopic view of the Orion Bar Astronomy and astrophysics (Berlin), 2023-10 [Peer Reviewed Journal] 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 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 2331-8422 ;EISSN: 1432-0746 ;DOI: 10.48550/arxiv.2310.08720 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
8	Material Type: Article	PDRs4All IV. An embarrassment of riches: Aromatic infrared bands in the Orion Bar Astronomy and astrophysics (Berlin), 2023-09 [Peer Reviewed Journal] 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 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 2331-8422 ;EISSN: 1432-0746 ;DOI: 10.48550/arxiv.2308.16733 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
9	Material Type: Article	An ALMA Glimpse of Dense Molecular Filaments Associated with High-mass Protostellar Systems in the Large Magellanic Cloud The Astrophysical journal, 2023-08, Vol.955 (1) [Peer Reviewed Journal] Copyright Determination: MAY_INCLUDE_COPYRIGHT_MATERIAL ;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 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;EISSN: 2331-8422 ;DOI: 10.48550/arXiv.2308.05568 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
10	Material Type: Article	PDRs4All II: JWST's NIR and MIR imaging view of the Orion Nebula arXiv.org, 2023-09 [Peer Reviewed Journal] 2023. This work is published under http://creativecommons.org/publicdomain/zero/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://creativecommons.org/publicdomain/zero/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.2308.16732 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
11	Material Type: Article	A global view on star formation: The GLOSTAR Galactic plane survey. IX. Radio Source Catalog III: 2<l<28, 36<l<40, 56<l<60 and \|b\|<1, VLA B-configuration arXiv.org, 2023-10 [Peer Reviewed Journal] 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.2310.09777 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
12	Material Type: Article	ALMA-IMF VIII -- Combination of Interferometric Continuum Images with Single-Dish Surveys and Structural Analysis of Six Protoclusters The Astrophysical journal. Supplement series, 2023-10 [Peer Reviewed Journal] 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 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0067-0049 ;EISSN: 2331-8422 ;EISSN: 1538-4365 ;DOI: 10.48550/arxiv.2310.13872 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
13	$3D chemical structure of the diffuse turbulent ISM II -- Origin of CH$^+$, new solution to an 80 years mystery$ $3D chemical structure of the diffuse turbulent ISM II -- Origin of CH$^+$, new solution to an 80 years mystery$ Material Type: Article	3D chemical structure of the diffuse turbulent ISM II -- Origin of CH$^+$, new solution to an 80 years mystery Astronomy and astrophysics (Berlin), 2022-09 [Peer Reviewed Journal] 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 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 2331-8422 ;EISSN: 1432-0746 ;DOI: 10.48550/arxiv.2209.10196 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
14	Material Type: Article	The GALAH Survey: Chemical Clocks Monthly notices of the Royal Astronomical Society, 2020-11, Vol.517 (4), p.5325 [Peer Reviewed Journal] 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 ;ISSN: 1365-2966 ;EISSN: 2331-8422 ;EISSN: 1365-2966 ;DOI: 10.48550/arxiv.2011.13745 Full text available View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
15	Material Type: Article	Understanding the chemistry of the young stellar object G29.862-0.0044 http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2406.02358 Digital Resources/Online E-Resources View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
16	Material Type: Article	Local versus global environment: the suppression of star formation in the vicinity of galaxy clusters http://creativecommons.org/licenses/by/4.0 ;DOI: 10.48550/arxiv.2406.02196 Digital Resources/Online E-Resources View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
17	Material Type: Article	Observation of HI around three satellite galaxies of the M31 with the FAST: Andromeda II, NGC 205, and NGC 185 http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2406.02215 Digital Resources/Online E-Resources View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
18	$The MAGPI Survey: Massive slow rotator population in place by $z \sim 0.3$ $The MAGPI Survey: Massive slow rotator population in place by $z \sim 0.3$ Material Type: Article	The MAGPI Survey: Massive slow rotator population in place by $z \sim 0.3 http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2406.02185 Digital Resources/Online E-Resources View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
19	Material Type: Article	UV Cooling via O VI Emission in the Superwind of M82 Observed with the Far Ultraviolet Spectroscopic Explorer (FUSE) http://creativecommons.org/licenses/by/4.0 ;DOI: 10.48550/arxiv.2406.01742 Digital Resources/Online E-Resources View Online Details Recommendations Reviews Times Cited External Links Citations Cited by
20	Material Type: Article	Feedback in Emerging extragAlactic Star clusTers, FEAST: JWST spots PAH destruction in NGC 628 during the emerging phase of star formation http://creativecommons.org/licenses/by/4.0 ;DOI: 10.48550/arxiv.2406.01666 Digital Resources/Online E-Resources View Online Details Recommendations Reviews Times Cited External Links Citations Cited by

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Results 1 - 20 of 169,251 for All Library Resources

PDRs4All VII. The 3.3 $\mu$m aromatic infrared band as a tracer of physical properties of the ISM in galaxies

http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2402.16535

Time variability of ultra-fast BAL outflows using SALT: C IV absorption depth based analysis

http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 1745-3933 ;EISSN: 1745-3933 ;DOI: 10.48550/arxiv.2312.17320

PDRs4All VI: Probing the Photochemical Evolution of PAHs in the Orion Bar Using Machine Learning Techniques

PDRs4All. V. Modelling the dust evolution across the illuminated edge of the Orion Bar

ALMA-IMF IX: Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters

GOODS-ALMA 2.0: Last gigayear star formation histories of the so-called starbursts within the main sequence

PDRs4All III: JWST's NIR spectroscopic view of the Orion Bar

PDRs4All IV. An embarrassment of riches: Aromatic infrared bands in the Orion Bar

An ALMA Glimpse of Dense Molecular Filaments Associated with High-mass Protostellar Systems in the Large Magellanic Cloud

PDRs4All II: JWST's NIR and MIR imaging view of the Orion Nebula

A global view on star formation: The GLOSTAR Galactic plane survey. IX. Radio Source Catalog III: 2<l<28, 36<l<40, 56<l<60 and |b|<1, VLA B-configuration

ALMA-IMF VIII -- Combination of Interferometric Continuum Images with Single-Dish Surveys and Structural Analysis of Six Protoclusters

3D chemical structure of the diffuse turbulent ISM II -- Origin of CH\(^+\), new solution to an 80 years mystery

The GALAH Survey: Chemical Clocks

Understanding the chemistry of the young stellar object G29.862-0.0044

http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2406.02358

Local versus global environment: the suppression of star formation in the vicinity of galaxy clusters

http://creativecommons.org/licenses/by/4.0 ;DOI: 10.48550/arxiv.2406.02196

Observation of HI around three satellite galaxies of the M31 with the FAST: Andromeda II, NGC 205, and NGC 185

http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2406.02215

The MAGPI Survey: Massive slow rotator population in place by $z \sim 0.3

http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2406.02185

UV Cooling via O VI Emission in the Superwind of M82 Observed with the Far Ultraviolet Spectroscopic Explorer (FUSE)

http://creativecommons.org/licenses/by/4.0 ;DOI: 10.48550/arxiv.2406.01742

Feedback in Emerging extragAlactic Star clusTers, FEAST: JWST spots PAH destruction in NGC 628 during the emerging phase of star formation

http://creativecommons.org/licenses/by/4.0 ;DOI: 10.48550/arxiv.2406.01666

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http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2402.16535

http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 1745-3933 ;EISSN: 1745-3933 ;DOI: 10.48550/arxiv.2312.17320

http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2406.02358

http://creativecommons.org/licenses/by/4.0 ;DOI: 10.48550/arxiv.2406.02196

http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2406.02215

http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;DOI: 10.48550/arxiv.2406.02185

http://creativecommons.org/licenses/by/4.0 ;DOI: 10.48550/arxiv.2406.01742

http://creativecommons.org/licenses/by/4.0 ;DOI: 10.48550/arxiv.2406.01666

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