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PAH Marks the Spot: Digging for Buried Clusters in Nearby Star-forming Galaxies

  • Authors: Gabrielle B. Graham, Daniel A. Dale, Chase L. Smith, Elisabeth Brann, Kaycee D. Conder, Samuel Crowe, Sumitra Dhileepkumar, Nicole A. Imming, Emilio Mendez, Zachary Pleska, Kelsey Sako, Amirnezam Amiri, Ashley T. Barnes, Médéric Boquien, Rupali Chandar, Ryan Chown, Oleg Y. Gnedin, Kathryn Grasha, Stephen Hannon, Hamid Hassani, Rémy Indebetouw, Hwihyun Kim, Jaeyeon Kim, Hannah Koziol, Kirsten L. Larson, Janice C. Lee, Adam K. Leroy, Elias K. Oakes, M. Jimena Rodríguez, Erik Rosolowsky, Karin Sandstrom, Eva Schinnerer, Jessica Sutter, David A. Thilker, Leonardo Ubeda, Bradley C. Whitmore, Tony D. Weinbeck, Thomas G. Williams, Aida Wofford, J. Eduardo Méndez-Delgado, Qiushi Chris Tian

Gabrielle B. Graham et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 3.

Number of embedded cluster candidates vs. global star formation properties. Values for each galaxy are in Table 1, and embedded cluster candidate counts from this study are in Table 4. Left: ﹩{{\rm{log}}}_{10}({\rm{SFR}})﹩ vs. number of embedded cluster candidates. Right: ﹩{{\rm{log}}}_{10}({\rm{sSFR}})﹩ vs. number of embedded cluster candidates. The black line in each plot shows the linear fit to the data with the ±1σ region of the fit in light gray. We exclude NGC 2997 and NGC 1097 in fitting due to a lack of wide coverage. The number of embedded cluster candidates positively correlates with each of these properties.

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