PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365
- Autores
- Whitmore, Bradley C.; Chandar, Rupali; Rodriguez, Maria Jimena; Lee, Janice C.; Emsellem, Eric; Floyd, Matthew; Kim, Hwihyun; Kruijssen, J. M. Diederik; Mok, Angus; Sormani, Mattia C.; Boquien, Médéric; Dale, Daniel A.; Faesi, Christopher M.; Henny, Kiana F.; Hannon, Stephen; Thilker, David A.; White, Richard L.; Barnes, Ashley T.; Bigiel, F.; Chevance, Mélanie; Henshaw, Jonathan D.; Klessen, Ralf S.; Leroy, Adam K.; Liu, Daizhong; Maschmann, Daniel; Meidt, Sharon E.; Rosolowsky, Erik; Schinnerer, Eva; Sun, Jiayi; Watkins, Elizabeth J.; Williams, Thomas G.
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- A primary new capability of JWST is the ability to penetrate the dust in star-forming galaxies to identify and study the properties of young star clusters that remain embedded in dust and gas. In this Letter we combine new infrared images taken with JWST with our optical Hubble Space Telescope (HST) images of the starbursting barred (Seyfert2) spiral galaxy NGC 1365. We find that this galaxy has the richest population of massive young clusters of any known galaxy within 30 Mpc, with ∼30 star clusters that are more massive than 106 M ⊙ and younger than 10 Myr. Sixteen of these clusters are newly discovered from our JWST observations. An examination of the optical images reveals that 4 of 30 (∼13%) are so deeply embedded that they cannot be seen in the Hubble I band (A V ≳ 10 mag), and that 11 of 30 (∼37%) are missing in the HST B band, so age and mass estimates from optical measurements alone are challenging. These numbers suggest that massive clusters in NGC 1365 remain completely obscured in the visible for ∼1.3 ± 0.7 Myr and are either completely or partially obscured for ∼3.7 ± 1.1 Myr. We also use the JWST observations to gain new insights into the triggering of star cluster formation by the collision of gas and dust streamers with gas and dust in the bar. The JWST images reveal previously unknown structures (e.g., bridges and overshoot regions from stars that form in the bar) that help us better understand the orbital dynamics of barred galaxies and associated star-forming rings. Finally, we note that the excellent spatial resolution of the NIRCAM F200W filter provides a better way to separate barely resolved compact clusters from individual stars based on their sizes.
Fil: Whitmore, Bradley C.. Space Telescope Science Institute; Estados Unidos
Fil: Chandar, Rupali. The University of Toledo; Estados Unidos
Fil: Rodriguez, Maria Jimena. University of Arizona; Estados Unidos. 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
Fil: Lee, Janice C.. Gemini Observatory; Estados Unidos
Fil: Emsellem, Eric. European Southern Observatory; Alemania
Fil: Floyd, Matthew. The University of Toledo; Estados Unidos
Fil: Kim, Hwihyun. Gemini Observatory; Estados Unidos
Fil: Kruijssen, J. M. Diederik. Research DAO; Estados Unidos
Fil: Mok, Angus. The Ontario College Of Art And Design University; Canadá
Fil: Sormani, Mattia C.. Astronomisches Rechen-institut; Alemania
Fil: Boquien, Médéric. Universidad de Antofagasta; Chile
Fil: Dale, Daniel A.. University of Wyoming; Estados Unidos
Fil: Faesi, Christopher M.. University of Connecticut; Estados Unidos
Fil: Henny, Kiana F.. University of Wyoming; Estados Unidos
Fil: Hannon, Stephen. University of California; Estados Unidos
Fil: Thilker, David A.. University Johns Hopkins; Estados Unidos
Fil: White, Richard L.. Space Telescope Science Institute; Estados Unidos
Fil: Barnes, Ashley T.. Universitat Bonn; Alemania
Fil: Bigiel, F.. Universitat Bonn; Alemania
Fil: Chevance, Mélanie. Universität Heidelberg; Alemania
Fil: Henshaw, Jonathan D.. Liverpool John Moores University; Reino Unido
Fil: Klessen, Ralf S.. Universität Heidelberg; Alemania
Fil: Leroy, Adam K.. Ohio State University; Estados Unidos
Fil: Liu, Daizhong. Max Planck Institute For Extraterrestrial Physics; Alemania
Fil: Maschmann, Daniel. University of Arizona; Estados Unidos. Université Pierre et Marie Curie; Francia
Fil: Meidt, Sharon E.. University of Ghent; Bélgica
Fil: Rosolowsky, Erik. University of Alberta; Canadá
Fil: Schinnerer, Eva. Max Planck Institute For Astronomy; Alemania
Fil: Sun, Jiayi. Linstitut Canadien Dastrophysique Théorique; Canadá
Fil: Watkins, Elizabeth J.. Astronomisches Rechen-institut; Alemania
Fil: Williams, Thomas G.. Max Planck Institute For Astronomy; Alemania - Materia
-
BARRED SPIRAL GALAXIES
YOUNG STAR CLUSTERS
YOUNG MASSIVE STAR CLUSTERS - 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:11336/234299
Ver los metadatos del registro completo
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PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365Whitmore, Bradley C.Chandar, RupaliRodriguez, Maria JimenaLee, Janice C.Emsellem, EricFloyd, MatthewKim, HwihyunKruijssen, J. M. DiederikMok, AngusSormani, Mattia C.Boquien, MédéricDale, Daniel A.Faesi, Christopher M.Henny, Kiana F.Hannon, StephenThilker, David A.White, Richard L.Barnes, Ashley T.Bigiel, F.Chevance, MélanieHenshaw, Jonathan D.Klessen, Ralf S.Leroy, Adam K.Liu, DaizhongMaschmann, DanielMeidt, Sharon E.Rosolowsky, ErikSchinnerer, EvaSun, JiayiWatkins, Elizabeth J.Williams, Thomas G.BARRED SPIRAL GALAXIESYOUNG STAR CLUSTERSYOUNG MASSIVE STAR CLUSTERShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A primary new capability of JWST is the ability to penetrate the dust in star-forming galaxies to identify and study the properties of young star clusters that remain embedded in dust and gas. In this Letter we combine new infrared images taken with JWST with our optical Hubble Space Telescope (HST) images of the starbursting barred (Seyfert2) spiral galaxy NGC 1365. We find that this galaxy has the richest population of massive young clusters of any known galaxy within 30 Mpc, with ∼30 star clusters that are more massive than 106 M ⊙ and younger than 10 Myr. Sixteen of these clusters are newly discovered from our JWST observations. An examination of the optical images reveals that 4 of 30 (∼13%) are so deeply embedded that they cannot be seen in the Hubble I band (A V ≳ 10 mag), and that 11 of 30 (∼37%) are missing in the HST B band, so age and mass estimates from optical measurements alone are challenging. These numbers suggest that massive clusters in NGC 1365 remain completely obscured in the visible for ∼1.3 ± 0.7 Myr and are either completely or partially obscured for ∼3.7 ± 1.1 Myr. We also use the JWST observations to gain new insights into the triggering of star cluster formation by the collision of gas and dust streamers with gas and dust in the bar. The JWST images reveal previously unknown structures (e.g., bridges and overshoot regions from stars that form in the bar) that help us better understand the orbital dynamics of barred galaxies and associated star-forming rings. Finally, we note that the excellent spatial resolution of the NIRCAM F200W filter provides a better way to separate barely resolved compact clusters from individual stars based on their sizes.Fil: Whitmore, Bradley C.. Space Telescope Science Institute; Estados UnidosFil: Chandar, Rupali. The University of Toledo; Estados UnidosFil: Rodriguez, Maria Jimena. University of Arizona; Estados Unidos. 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; ArgentinaFil: Lee, Janice C.. Gemini Observatory; Estados UnidosFil: Emsellem, Eric. European Southern Observatory; AlemaniaFil: Floyd, Matthew. The University of Toledo; Estados UnidosFil: Kim, Hwihyun. Gemini Observatory; Estados UnidosFil: Kruijssen, J. M. Diederik. Research DAO; Estados UnidosFil: Mok, Angus. The Ontario College Of Art And Design University; CanadáFil: Sormani, Mattia C.. Astronomisches Rechen-institut; AlemaniaFil: Boquien, Médéric. Universidad de Antofagasta; ChileFil: Dale, Daniel A.. University of Wyoming; Estados UnidosFil: Faesi, Christopher M.. University of Connecticut; Estados UnidosFil: Henny, Kiana F.. University of Wyoming; Estados UnidosFil: Hannon, Stephen. University of California; Estados UnidosFil: Thilker, David A.. University Johns Hopkins; Estados UnidosFil: White, Richard L.. Space Telescope Science Institute; Estados UnidosFil: Barnes, Ashley T.. Universitat Bonn; AlemaniaFil: Bigiel, F.. Universitat Bonn; AlemaniaFil: Chevance, Mélanie. Universität Heidelberg; AlemaniaFil: Henshaw, Jonathan D.. Liverpool John Moores University; Reino UnidoFil: Klessen, Ralf S.. Universität Heidelberg; AlemaniaFil: Leroy, Adam K.. Ohio State University; Estados UnidosFil: Liu, Daizhong. Max Planck Institute For Extraterrestrial Physics; AlemaniaFil: Maschmann, Daniel. University of Arizona; Estados Unidos. Université Pierre et Marie Curie; FranciaFil: Meidt, Sharon E.. University of Ghent; BélgicaFil: Rosolowsky, Erik. University of Alberta; CanadáFil: Schinnerer, Eva. Max Planck Institute For Astronomy; AlemaniaFil: Sun, Jiayi. Linstitut Canadien Dastrophysique Théorique; CanadáFil: Watkins, Elizabeth J.. Astronomisches Rechen-institut; AlemaniaFil: Williams, Thomas G.. Max Planck Institute For Astronomy; AlemaniaIOP Publishing2023-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/234299Whitmore, Bradley C.; Chandar, Rupali; Rodriguez, Maria Jimena; Lee, Janice C.; Emsellem, Eric; et al.; PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365; IOP Publishing; Astrophysical Journal Letters; 944; 2; 2-2023; 1-132041-82052041-8213CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/2041-8213/acae94info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2041-8213/acae94info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:02:31Zoai:ri.conicet.gov.ar:11336/234299instacron: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 10:02:31.781CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365 |
| title |
PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365 |
| spellingShingle |
PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365 Whitmore, Bradley C. BARRED SPIRAL GALAXIES YOUNG STAR CLUSTERS YOUNG MASSIVE STAR CLUSTERS |
| title_short |
PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365 |
| title_full |
PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365 |
| title_fullStr |
PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365 |
| title_full_unstemmed |
PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365 |
| title_sort |
PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365 |
| dc.creator.none.fl_str_mv |
Whitmore, Bradley C. Chandar, Rupali Rodriguez, Maria Jimena Lee, Janice C. Emsellem, Eric Floyd, Matthew Kim, Hwihyun Kruijssen, J. M. Diederik Mok, Angus Sormani, Mattia C. Boquien, Médéric Dale, Daniel A. Faesi, Christopher M. Henny, Kiana F. Hannon, Stephen Thilker, David A. White, Richard L. Barnes, Ashley T. Bigiel, F. Chevance, Mélanie Henshaw, Jonathan D. Klessen, Ralf S. Leroy, Adam K. Liu, Daizhong Maschmann, Daniel Meidt, Sharon E. Rosolowsky, Erik Schinnerer, Eva Sun, Jiayi Watkins, Elizabeth J. Williams, Thomas G. |
| author |
Whitmore, Bradley C. |
| author_facet |
Whitmore, Bradley C. Chandar, Rupali Rodriguez, Maria Jimena Lee, Janice C. Emsellem, Eric Floyd, Matthew Kim, Hwihyun Kruijssen, J. M. Diederik Mok, Angus Sormani, Mattia C. Boquien, Médéric Dale, Daniel A. Faesi, Christopher M. Henny, Kiana F. Hannon, Stephen Thilker, David A. White, Richard L. Barnes, Ashley T. Bigiel, F. Chevance, Mélanie Henshaw, Jonathan D. Klessen, Ralf S. Leroy, Adam K. Liu, Daizhong Maschmann, Daniel Meidt, Sharon E. Rosolowsky, Erik Schinnerer, Eva Sun, Jiayi Watkins, Elizabeth J. Williams, Thomas G. |
| author_role |
author |
| author2 |
Chandar, Rupali Rodriguez, Maria Jimena Lee, Janice C. Emsellem, Eric Floyd, Matthew Kim, Hwihyun Kruijssen, J. M. Diederik Mok, Angus Sormani, Mattia C. Boquien, Médéric Dale, Daniel A. Faesi, Christopher M. Henny, Kiana F. Hannon, Stephen Thilker, David A. White, Richard L. Barnes, Ashley T. Bigiel, F. Chevance, Mélanie Henshaw, Jonathan D. Klessen, Ralf S. Leroy, Adam K. Liu, Daizhong Maschmann, Daniel Meidt, Sharon E. Rosolowsky, Erik Schinnerer, Eva Sun, Jiayi Watkins, Elizabeth J. Williams, Thomas G. |
| 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 author |
| dc.subject.none.fl_str_mv |
BARRED SPIRAL GALAXIES YOUNG STAR CLUSTERS YOUNG MASSIVE STAR CLUSTERS |
| topic |
BARRED SPIRAL GALAXIES YOUNG STAR CLUSTERS YOUNG MASSIVE STAR CLUSTERS |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
A primary new capability of JWST is the ability to penetrate the dust in star-forming galaxies to identify and study the properties of young star clusters that remain embedded in dust and gas. In this Letter we combine new infrared images taken with JWST with our optical Hubble Space Telescope (HST) images of the starbursting barred (Seyfert2) spiral galaxy NGC 1365. We find that this galaxy has the richest population of massive young clusters of any known galaxy within 30 Mpc, with ∼30 star clusters that are more massive than 106 M ⊙ and younger than 10 Myr. Sixteen of these clusters are newly discovered from our JWST observations. An examination of the optical images reveals that 4 of 30 (∼13%) are so deeply embedded that they cannot be seen in the Hubble I band (A V ≳ 10 mag), and that 11 of 30 (∼37%) are missing in the HST B band, so age and mass estimates from optical measurements alone are challenging. These numbers suggest that massive clusters in NGC 1365 remain completely obscured in the visible for ∼1.3 ± 0.7 Myr and are either completely or partially obscured for ∼3.7 ± 1.1 Myr. We also use the JWST observations to gain new insights into the triggering of star cluster formation by the collision of gas and dust streamers with gas and dust in the bar. The JWST images reveal previously unknown structures (e.g., bridges and overshoot regions from stars that form in the bar) that help us better understand the orbital dynamics of barred galaxies and associated star-forming rings. Finally, we note that the excellent spatial resolution of the NIRCAM F200W filter provides a better way to separate barely resolved compact clusters from individual stars based on their sizes. Fil: Whitmore, Bradley C.. Space Telescope Science Institute; Estados Unidos Fil: Chandar, Rupali. The University of Toledo; Estados Unidos Fil: Rodriguez, Maria Jimena. University of Arizona; Estados Unidos. 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 Fil: Lee, Janice C.. Gemini Observatory; Estados Unidos Fil: Emsellem, Eric. European Southern Observatory; Alemania Fil: Floyd, Matthew. The University of Toledo; Estados Unidos Fil: Kim, Hwihyun. Gemini Observatory; Estados Unidos Fil: Kruijssen, J. M. Diederik. Research DAO; Estados Unidos Fil: Mok, Angus. The Ontario College Of Art And Design University; Canadá Fil: Sormani, Mattia C.. Astronomisches Rechen-institut; Alemania Fil: Boquien, Médéric. Universidad de Antofagasta; Chile Fil: Dale, Daniel A.. University of Wyoming; Estados Unidos Fil: Faesi, Christopher M.. University of Connecticut; Estados Unidos Fil: Henny, Kiana F.. University of Wyoming; Estados Unidos Fil: Hannon, Stephen. University of California; Estados Unidos Fil: Thilker, David A.. University Johns Hopkins; Estados Unidos Fil: White, Richard L.. Space Telescope Science Institute; Estados Unidos Fil: Barnes, Ashley T.. Universitat Bonn; Alemania Fil: Bigiel, F.. Universitat Bonn; Alemania Fil: Chevance, Mélanie. Universität Heidelberg; Alemania Fil: Henshaw, Jonathan D.. Liverpool John Moores University; Reino Unido Fil: Klessen, Ralf S.. Universität Heidelberg; Alemania Fil: Leroy, Adam K.. Ohio State University; Estados Unidos Fil: Liu, Daizhong. Max Planck Institute For Extraterrestrial Physics; Alemania Fil: Maschmann, Daniel. University of Arizona; Estados Unidos. Université Pierre et Marie Curie; Francia Fil: Meidt, Sharon E.. University of Ghent; Bélgica Fil: Rosolowsky, Erik. University of Alberta; Canadá Fil: Schinnerer, Eva. Max Planck Institute For Astronomy; Alemania Fil: Sun, Jiayi. Linstitut Canadien Dastrophysique Théorique; Canadá Fil: Watkins, Elizabeth J.. Astronomisches Rechen-institut; Alemania Fil: Williams, Thomas G.. Max Planck Institute For Astronomy; Alemania |
| description |
A primary new capability of JWST is the ability to penetrate the dust in star-forming galaxies to identify and study the properties of young star clusters that remain embedded in dust and gas. In this Letter we combine new infrared images taken with JWST with our optical Hubble Space Telescope (HST) images of the starbursting barred (Seyfert2) spiral galaxy NGC 1365. We find that this galaxy has the richest population of massive young clusters of any known galaxy within 30 Mpc, with ∼30 star clusters that are more massive than 106 M ⊙ and younger than 10 Myr. Sixteen of these clusters are newly discovered from our JWST observations. An examination of the optical images reveals that 4 of 30 (∼13%) are so deeply embedded that they cannot be seen in the Hubble I band (A V ≳ 10 mag), and that 11 of 30 (∼37%) are missing in the HST B band, so age and mass estimates from optical measurements alone are challenging. These numbers suggest that massive clusters in NGC 1365 remain completely obscured in the visible for ∼1.3 ± 0.7 Myr and are either completely or partially obscured for ∼3.7 ± 1.1 Myr. We also use the JWST observations to gain new insights into the triggering of star cluster formation by the collision of gas and dust streamers with gas and dust in the bar. The JWST images reveal previously unknown structures (e.g., bridges and overshoot regions from stars that form in the bar) that help us better understand the orbital dynamics of barred galaxies and associated star-forming rings. Finally, we note that the excellent spatial resolution of the NIRCAM F200W filter provides a better way to separate barely resolved compact clusters from individual stars based on their sizes. |
| 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/11336/234299 Whitmore, Bradley C.; Chandar, Rupali; Rodriguez, Maria Jimena; Lee, Janice C.; Emsellem, Eric; et al.; PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365; IOP Publishing; Astrophysical Journal Letters; 944; 2; 2-2023; 1-13 2041-8205 2041-8213 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/234299 |
| identifier_str_mv |
Whitmore, Bradley C.; Chandar, Rupali; Rodriguez, Maria Jimena; Lee, Janice C.; Emsellem, Eric; et al.; PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365; IOP Publishing; Astrophysical Journal Letters; 944; 2; 2-2023; 1-13 2041-8205 2041-8213 CONICET Digital CONICET |
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