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dc.contributor.authorCosta, Allison H.
dc.contributor.authorJohnson, Kelsey E.
dc.contributor.authorIndebetouw, Remy
dc.contributor.authorFinn, Molly K.
dc.contributor.authorBrogan, Crystal L.
dc.contributor.authorReines, Amy
dc.date.accessioned2022-09-21T21:53:36Z
dc.date.available2022-09-21T21:53:36Z
dc.date.issued2021-09
dc.identifier.citationCosta, A. H., Johnson, K. E., Indebetouw, R., Finn, M. K., Brogan, C. L., & Reines, A. (2021). Toward a More Complex Understanding of Natal Super Star Clusters with Multiwavelength Observations. The Astrophysical Journal, 918(2), 76.en_US
dc.identifier.issn0004-637X
dc.identifier.urihttps://scholarworks.montana.edu/xmlui/handle/1/17206
dc.description.abstractHenize 2–10 (He 2–10) is a nearby (D = 9 Mpc) starbursting blue compact dwarf galaxy that boasts a high star formation rate and a low-luminosity active galactic nucleus. He 2–10 is also one of the first galaxies in which embedded super star clusters (SSCs) were discovered. SSCs are massive, compact star clusters that will impact their host galaxies dramatically when their massive stars evolve. Here, we discuss radio, submillimeter, and infrared observations of He 2–10 from 1.87 μm to 6 cm in high angular resolution (∼0.3''), which allows us to disentangle individual clusters from aggregate complexes as identified at lower resolution. These results indicate the importance of spatial resolution to characterize SSCs, as low resolution studies of SSCs average over aggregate complexes that may host SSCs at different stages of evolution. We explore the thermal, nonthermal, and dust emission associated with the clusters along with dense molecular tracers to construct a holistic review of the natal SSCs that have yet to dramatically disrupt their parent molecular clouds. We assess the production rate of ionizing photons, extinction, total mass, and the star formation efficiency (SFE) associated with the clusters. Notably, we find that the SFE for the some of the natal clusters is high (>70%), which suggests that these clusters could remain bound even after the gas is dispersed from the system from stellar feedback mechanisms. If they remain bound, these SSCs could survive to become objects indistinguishable from globular clusters.en_US
dc.language.isoen_USen_US
dc.publisherAmerican Astronomical Societyen_US
dc.rightscc-byen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.subjectinterstellar mediumen_US
dc.subjectstar clustersen_US
dc.subjectH n regionsen_US
dc.subjectstar formationen_US
dc.subjectblue compact dwarf galaxiesen_US
dc.titleToward a More Complex Understanding of Natal Super Star Clusters with Multiwavelength Observationsen_US
dc.typeArticleen_US
mus.citation.extentfirstpage918en_US
mus.citation.extentlastpage2en_US
mus.citation.journaltitleThe Astrophysical Journalen_US
mus.identifier.doi10.3847/1538-4357/ac0e93en_US
mus.relation.collegeCollege of Letters & Scienceen_US
mus.relation.departmentPhysics.en_US
mus.relation.universityMontana State University - Bozemanen_US
mus.data.thumbpage3en_US


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