The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS
- Autores
- Lee, Janice C.; Sandstrom, Karin M.; Leroy, Adam K.; Thilker, David A.; Schinnerer, Eva; Rosolowsky, Erik; Larson, Kirsten L.; Egorov, Oleg V.; Williams, Thomas G.; Schmidt, Judy; Emsellem, Eric; Anand, Gagandeep S.; Barnes, Ashley T.; Belfiore, Francesco; Beslik, Ivana; Bigiel, Frank; Blanc, Guillermo A.; Bolatto, Alberto D.; Boquien, Médéric; Brok, Jakob den; Cao, Yixian; Chandar, Rupali; Chastenet, Jérémy; Chevance, Mélanie; Congiu, Enrico; Eibensteiner, Cosima; Glover, Simon C. O.; Hassani, Hamid; Henshaw, Jonathan D.; Rodriguez, Maria Jimena
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The PHANGS collaboration has been building a reference data set for the multiscale, multiphase study of star formation and the interstellar medium (ISM) in nearby galaxies. With the successful launch and commissioning of JWST, we can now obtain high-resolution infrared imaging to probe the youngest stellar populations and dust emission on the scales of star clusters and molecular clouds (∼5-50 pc). In Cycle 1, PHANGS is conducting an eight-band imaging survey from 2 to 21 μm of 19 nearby spiral galaxies. Optical integral field spectroscopy, CO(2-1) mapping, and UV-optical imaging for all 19 galaxies have been obtained through large programs with ALMA, VLT-MUSE, and Hubble. PHANGS-JWST enables a full inventory of star formation, accurate measurement of the mass and age of star clusters, identification of the youngest embedded stellar populations, and characterization of the physical state of small dust grains. When combined with Hubble catalogs of ∼10,000 star clusters, MUSE spectroscopic mapping of ∼20,000 H ii regions, and ∼12,000 ALMA-identified molecular clouds, it becomes possible to measure the timescales and efficiencies of the earliest phases of star formation and feedback, build an empirical model of the dependence of small dust grain properties on local ISM conditions, and test our understanding of how dust-reprocessed starlight traces star formation activity, all across a diversity of galactic environments. Here we describe the PHANGS-JWST Treasury survey, present the remarkable imaging obtained in the first few months of science operations, and provide context for the initial results presented in the first series of PHANGS-JWST publications.
Fil: Lee, Janice C.. University of Arizona; Estados Unidos
Fil: Sandstrom, Karin M.. University of California; Estados Unidos
Fil: Leroy, Adam K.. Ohio State University; Estados Unidos
Fil: Thilker, David A.. University Johns Hopkins; Estados Unidos
Fil: Schinnerer, Eva. Max Planck Institute For Astronomy; Alemania
Fil: Rosolowsky, Erik. University of Alberta; Canadá
Fil: Larson, Kirsten L.. Space Telescope Science Institute; Estados Unidos
Fil: Egorov, Oleg V.. Zentrum für Astronomie der Universität Heidelberg; Alemania
Fil: Williams, Thomas G.. Max Planck Institute For Astronomy; Alemania
Fil: Schmidt, Judy. Michigan Technological University; Estados Unidos
Fil: Emsellem, Eric. European Southern Observatory; Alemania
Fil: Anand, Gagandeep S.. Space Telescope Science Institute; Estados Unidos
Fil: Barnes, Ashley T.. Universitat Bonn; Alemania
Fil: Belfiore, Francesco. Osservatorio Astrofisico Di Arcetri; Italia
Fil: Beslik, Ivana. Universitat Bonn; Alemania
Fil: Bigiel, Frank. Universitat Bonn; Alemania
Fil: Blanc, Guillermo A.. Universidad de Chile; Chile
Fil: Bolatto, Alberto D.. University of Maryland; Estados Unidos
Fil: Boquien, Médéric. Universidad de Antofagasta; Chile
Fil: Brok, Jakob den. Universitat Bonn; Alemania
Fil: Cao, Yixian. Max Planck Institute For Extraterrestrial Physics; Alemania
Fil: Chandar, Rupali. The University of Toledo; España
Fil: Chastenet, Jérémy. University of Ghent; Bélgica
Fil: Chevance, Mélanie. Universität Heidelberg; Alemania
Fil: Congiu, Enrico. Universidad de Chile; Chile
Fil: Eibensteiner, Cosima. Universitat Bonn; Alemania
Fil: Glover, Simon C. O.. Universität Heidelberg; Alemania
Fil: Hassani, Hamid. University of Alberta; Canadá
Fil: Henshaw, Jonathan D.. Max Planck Institute For Astronomy; Alemania
Fil: Rodriguez, Maria Jimena. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. University of Arizona; Estados Unidos - Materia
-
SPIRAL GALAXIES
SURVEYS
YOUNG STAR CLUSTERS
STAR FORMATION - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/234111
Ver los metadatos del registro completo
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The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieSLee, Janice C.Sandstrom, Karin M.Leroy, Adam K.Thilker, David A.Schinnerer, EvaRosolowsky, ErikLarson, Kirsten L.Egorov, Oleg V.Williams, Thomas G.Schmidt, JudyEmsellem, EricAnand, Gagandeep S.Barnes, Ashley T.Belfiore, FrancescoBeslik, IvanaBigiel, FrankBlanc, Guillermo A.Bolatto, Alberto D.Boquien, MédéricBrok, Jakob denCao, YixianChandar, RupaliChastenet, JérémyChevance, MélanieCongiu, EnricoEibensteiner, CosimaGlover, Simon C. O.Hassani, HamidHenshaw, Jonathan D.Rodriguez, Maria JimenaSPIRAL GALAXIESSURVEYSYOUNG STAR CLUSTERSSTAR FORMATIONhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The PHANGS collaboration has been building a reference data set for the multiscale, multiphase study of star formation and the interstellar medium (ISM) in nearby galaxies. With the successful launch and commissioning of JWST, we can now obtain high-resolution infrared imaging to probe the youngest stellar populations and dust emission on the scales of star clusters and molecular clouds (∼5-50 pc). In Cycle 1, PHANGS is conducting an eight-band imaging survey from 2 to 21 μm of 19 nearby spiral galaxies. Optical integral field spectroscopy, CO(2-1) mapping, and UV-optical imaging for all 19 galaxies have been obtained through large programs with ALMA, VLT-MUSE, and Hubble. PHANGS-JWST enables a full inventory of star formation, accurate measurement of the mass and age of star clusters, identification of the youngest embedded stellar populations, and characterization of the physical state of small dust grains. When combined with Hubble catalogs of ∼10,000 star clusters, MUSE spectroscopic mapping of ∼20,000 H ii regions, and ∼12,000 ALMA-identified molecular clouds, it becomes possible to measure the timescales and efficiencies of the earliest phases of star formation and feedback, build an empirical model of the dependence of small dust grain properties on local ISM conditions, and test our understanding of how dust-reprocessed starlight traces star formation activity, all across a diversity of galactic environments. Here we describe the PHANGS-JWST Treasury survey, present the remarkable imaging obtained in the first few months of science operations, and provide context for the initial results presented in the first series of PHANGS-JWST publications.Fil: Lee, Janice C.. University of Arizona; Estados UnidosFil: Sandstrom, Karin M.. University of California; Estados UnidosFil: Leroy, Adam K.. Ohio State University; Estados UnidosFil: Thilker, David A.. University Johns Hopkins; Estados UnidosFil: Schinnerer, Eva. Max Planck Institute For Astronomy; AlemaniaFil: Rosolowsky, Erik. University of Alberta; CanadáFil: Larson, Kirsten L.. Space Telescope Science Institute; Estados UnidosFil: Egorov, Oleg V.. Zentrum für Astronomie der Universität Heidelberg; AlemaniaFil: Williams, Thomas G.. Max Planck Institute For Astronomy; AlemaniaFil: Schmidt, Judy. Michigan Technological University; Estados UnidosFil: Emsellem, Eric. European Southern Observatory; AlemaniaFil: Anand, Gagandeep S.. Space Telescope Science Institute; Estados UnidosFil: Barnes, Ashley T.. Universitat Bonn; AlemaniaFil: Belfiore, Francesco. Osservatorio Astrofisico Di Arcetri; ItaliaFil: Beslik, Ivana. Universitat Bonn; AlemaniaFil: Bigiel, Frank. Universitat Bonn; AlemaniaFil: Blanc, Guillermo A.. Universidad de Chile; ChileFil: Bolatto, Alberto D.. University of Maryland; Estados UnidosFil: Boquien, Médéric. Universidad de Antofagasta; ChileFil: Brok, Jakob den. Universitat Bonn; AlemaniaFil: Cao, Yixian. Max Planck Institute For Extraterrestrial Physics; AlemaniaFil: Chandar, Rupali. The University of Toledo; EspañaFil: Chastenet, Jérémy. University of Ghent; BélgicaFil: Chevance, Mélanie. Universität Heidelberg; AlemaniaFil: Congiu, Enrico. Universidad de Chile; ChileFil: Eibensteiner, Cosima. Universitat Bonn; AlemaniaFil: Glover, Simon C. O.. Universität Heidelberg; AlemaniaFil: Hassani, Hamid. University of Alberta; CanadáFil: Henshaw, Jonathan D.. Max Planck Institute For Astronomy; AlemaniaFil: Rodriguez, Maria Jimena. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. University of Arizona; Estados UnidosAmerican Astronomical Society2023-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/234111Lee, Janice C.; Sandstrom, Karin M.; Leroy, Adam K.; Thilker, David A.; Schinnerer, Eva; et al.; The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS; American Astronomical Society; Astrophysical Journal Letters; 944; L17; 2-2023; 1-232041-82052041-8213CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/2041-8213/acaaaeinfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2041-8213/acaaaeinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:34:43Zoai:ri.conicet.gov.ar:11336/234111instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:34:43.807CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS |
| title |
The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS |
| spellingShingle |
The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS Lee, Janice C. SPIRAL GALAXIES SURVEYS YOUNG STAR CLUSTERS STAR FORMATION |
| title_short |
The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS |
| title_full |
The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS |
| title_fullStr |
The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS |
| title_full_unstemmed |
The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS |
| title_sort |
The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS |
| dc.creator.none.fl_str_mv |
Lee, Janice C. Sandstrom, Karin M. Leroy, Adam K. Thilker, David A. Schinnerer, Eva Rosolowsky, Erik Larson, Kirsten L. Egorov, Oleg V. Williams, Thomas G. Schmidt, Judy Emsellem, Eric Anand, Gagandeep S. Barnes, Ashley T. Belfiore, Francesco Beslik, Ivana Bigiel, Frank Blanc, Guillermo A. Bolatto, Alberto D. Boquien, Médéric Brok, Jakob den Cao, Yixian Chandar, Rupali Chastenet, Jérémy Chevance, Mélanie Congiu, Enrico Eibensteiner, Cosima Glover, Simon C. O. Hassani, Hamid Henshaw, Jonathan D. Rodriguez, Maria Jimena |
| author |
Lee, Janice C. |
| author_facet |
Lee, Janice C. Sandstrom, Karin M. Leroy, Adam K. Thilker, David A. Schinnerer, Eva Rosolowsky, Erik Larson, Kirsten L. Egorov, Oleg V. Williams, Thomas G. Schmidt, Judy Emsellem, Eric Anand, Gagandeep S. Barnes, Ashley T. Belfiore, Francesco Beslik, Ivana Bigiel, Frank Blanc, Guillermo A. Bolatto, Alberto D. Boquien, Médéric Brok, Jakob den Cao, Yixian Chandar, Rupali Chastenet, Jérémy Chevance, Mélanie Congiu, Enrico Eibensteiner, Cosima Glover, Simon C. O. Hassani, Hamid Henshaw, Jonathan D. Rodriguez, Maria Jimena |
| author_role |
author |
| author2 |
Sandstrom, Karin M. Leroy, Adam K. Thilker, David A. Schinnerer, Eva Rosolowsky, Erik Larson, Kirsten L. Egorov, Oleg V. Williams, Thomas G. Schmidt, Judy Emsellem, Eric Anand, Gagandeep S. Barnes, Ashley T. Belfiore, Francesco Beslik, Ivana Bigiel, Frank Blanc, Guillermo A. Bolatto, Alberto D. Boquien, Médéric Brok, Jakob den Cao, Yixian Chandar, Rupali Chastenet, Jérémy Chevance, Mélanie Congiu, Enrico Eibensteiner, Cosima Glover, Simon C. O. Hassani, Hamid Henshaw, Jonathan D. Rodriguez, Maria Jimena |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
SPIRAL GALAXIES SURVEYS YOUNG STAR CLUSTERS STAR FORMATION |
| topic |
SPIRAL GALAXIES SURVEYS YOUNG STAR CLUSTERS STAR FORMATION |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
The PHANGS collaboration has been building a reference data set for the multiscale, multiphase study of star formation and the interstellar medium (ISM) in nearby galaxies. With the successful launch and commissioning of JWST, we can now obtain high-resolution infrared imaging to probe the youngest stellar populations and dust emission on the scales of star clusters and molecular clouds (∼5-50 pc). In Cycle 1, PHANGS is conducting an eight-band imaging survey from 2 to 21 μm of 19 nearby spiral galaxies. Optical integral field spectroscopy, CO(2-1) mapping, and UV-optical imaging for all 19 galaxies have been obtained through large programs with ALMA, VLT-MUSE, and Hubble. PHANGS-JWST enables a full inventory of star formation, accurate measurement of the mass and age of star clusters, identification of the youngest embedded stellar populations, and characterization of the physical state of small dust grains. When combined with Hubble catalogs of ∼10,000 star clusters, MUSE spectroscopic mapping of ∼20,000 H ii regions, and ∼12,000 ALMA-identified molecular clouds, it becomes possible to measure the timescales and efficiencies of the earliest phases of star formation and feedback, build an empirical model of the dependence of small dust grain properties on local ISM conditions, and test our understanding of how dust-reprocessed starlight traces star formation activity, all across a diversity of galactic environments. Here we describe the PHANGS-JWST Treasury survey, present the remarkable imaging obtained in the first few months of science operations, and provide context for the initial results presented in the first series of PHANGS-JWST publications. Fil: Lee, Janice C.. University of Arizona; Estados Unidos Fil: Sandstrom, Karin M.. University of California; Estados Unidos Fil: Leroy, Adam K.. Ohio State University; Estados Unidos Fil: Thilker, David A.. University Johns Hopkins; Estados Unidos Fil: Schinnerer, Eva. Max Planck Institute For Astronomy; Alemania Fil: Rosolowsky, Erik. University of Alberta; Canadá Fil: Larson, Kirsten L.. Space Telescope Science Institute; Estados Unidos Fil: Egorov, Oleg V.. Zentrum für Astronomie der Universität Heidelberg; Alemania Fil: Williams, Thomas G.. Max Planck Institute For Astronomy; Alemania Fil: Schmidt, Judy. Michigan Technological University; Estados Unidos Fil: Emsellem, Eric. European Southern Observatory; Alemania Fil: Anand, Gagandeep S.. Space Telescope Science Institute; Estados Unidos Fil: Barnes, Ashley T.. Universitat Bonn; Alemania Fil: Belfiore, Francesco. Osservatorio Astrofisico Di Arcetri; Italia Fil: Beslik, Ivana. Universitat Bonn; Alemania Fil: Bigiel, Frank. Universitat Bonn; Alemania Fil: Blanc, Guillermo A.. Universidad de Chile; Chile Fil: Bolatto, Alberto D.. University of Maryland; Estados Unidos Fil: Boquien, Médéric. Universidad de Antofagasta; Chile Fil: Brok, Jakob den. Universitat Bonn; Alemania Fil: Cao, Yixian. Max Planck Institute For Extraterrestrial Physics; Alemania Fil: Chandar, Rupali. The University of Toledo; España Fil: Chastenet, Jérémy. University of Ghent; Bélgica Fil: Chevance, Mélanie. Universität Heidelberg; Alemania Fil: Congiu, Enrico. Universidad de Chile; Chile Fil: Eibensteiner, Cosima. Universitat Bonn; Alemania Fil: Glover, Simon C. O.. Universität Heidelberg; Alemania Fil: Hassani, Hamid. University of Alberta; Canadá Fil: Henshaw, Jonathan D.. Max Planck Institute For Astronomy; Alemania Fil: Rodriguez, Maria Jimena. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. University of Arizona; Estados Unidos |
| description |
The PHANGS collaboration has been building a reference data set for the multiscale, multiphase study of star formation and the interstellar medium (ISM) in nearby galaxies. With the successful launch and commissioning of JWST, we can now obtain high-resolution infrared imaging to probe the youngest stellar populations and dust emission on the scales of star clusters and molecular clouds (∼5-50 pc). In Cycle 1, PHANGS is conducting an eight-band imaging survey from 2 to 21 μm of 19 nearby spiral galaxies. Optical integral field spectroscopy, CO(2-1) mapping, and UV-optical imaging for all 19 galaxies have been obtained through large programs with ALMA, VLT-MUSE, and Hubble. PHANGS-JWST enables a full inventory of star formation, accurate measurement of the mass and age of star clusters, identification of the youngest embedded stellar populations, and characterization of the physical state of small dust grains. When combined with Hubble catalogs of ∼10,000 star clusters, MUSE spectroscopic mapping of ∼20,000 H ii regions, and ∼12,000 ALMA-identified molecular clouds, it becomes possible to measure the timescales and efficiencies of the earliest phases of star formation and feedback, build an empirical model of the dependence of small dust grain properties on local ISM conditions, and test our understanding of how dust-reprocessed starlight traces star formation activity, all across a diversity of galactic environments. Here we describe the PHANGS-JWST Treasury survey, present the remarkable imaging obtained in the first few months of science operations, and provide context for the initial results presented in the first series of PHANGS-JWST publications. |
| publishDate |
2023 |
| dc.date.none.fl_str_mv |
2023-02 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/234111 Lee, Janice C.; Sandstrom, Karin M.; Leroy, Adam K.; Thilker, David A.; Schinnerer, Eva; et al.; The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS; American Astronomical Society; Astrophysical Journal Letters; 944; L17; 2-2023; 1-23 2041-8205 2041-8213 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/234111 |
| identifier_str_mv |
Lee, Janice C.; Sandstrom, Karin M.; Leroy, Adam K.; Thilker, David A.; Schinnerer, Eva; et al.; The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS; American Astronomical Society; Astrophysical Journal Letters; 944; L17; 2-2023; 1-23 2041-8205 2041-8213 CONICET Digital CONICET |
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eng |
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eng |
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info:eu-repo/semantics/altIdentifier/doi/10.3847/2041-8213/acaaae info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2041-8213/acaaae |
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