Circumnuclear dust in luminous Early-type galaxies. i. sample properties and stellar luminosity models

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dc.contributor.authorDavidson, Jared R
dc.contributor.authorBaker, Andrew J
dc.contributor.authorBoizelle, Benjamin D
dc.date.accessioned2025-10-29T10:29:54Z
dc.date.available2025-10-29T10:29:54Z
dc.date.issued2024
dc.description.abstractDusty circumnuclear disks (CNDs) in luminous early-type galaxies (ETGs) show regular, dynamically cold molecular gas kinematics. For a growing number of ETGs, Atacama Large Millimeter/sub-millimeter Array (ALMA) CO imaging and detailed gas-dynamical modeling facilitate moderate-to-high precision black hole (BH) mass (MBH) determinations. From the ALMA archive, we identified a subset of 26 ETGs with estimated MBH/Me  108 to a few × 109 and clean CO kinematics but that previously did not have sufficiently high-angularresolution near-IR observations to mitigate dust obscuration when constructing stellar luminosity models. We present new optical and near-IR Hubble Space Telescope (HST) images of this sample to supplement the archival HST data, detailing the sample properties and data-analysis techniques. After masking the most apparent dust features, we measure stellar surface-brightness profiles and model the luminosities using the multi-Gaussian expansion (MGE) formalism. Some of these MGEs have already been used in CO dynamical modeling efforts to secure quality MBH determinations, and the remaining ETG targets here are expected to significantly improve the high-mass end of the current BH census, facilitating new scrutiny of local BH mass–host galaxy scaling relationships. We also explore stellar isophotal behavior and general dust properties, finding these CNDs generally become optically thick in the near-IR (AH  1 mag). These CNDs are typically well aligned with the larger-scale stellar photometric axes, with a few notable exceptions. Uncertain dust impact on the MGE often dominates the BH mass error budget, so extensions of this work will focus on constraining CND dust attenuation.
dc.identifier.citationDavidson, J.R., Boizelle, B.D., Walsh, J.L., Barth, A.J., Rasmussen, E., Baker, A.J., Buote, D.A., Darling, J., Ho, L.C., Kabasares, K.M. and Cohn, J.H., 2024. Circumnuclear Dust in Luminous Early-type Galaxies. I. Sample Properties and Stellar Luminosity Models. The Astrophysical Journal, 972(1), p.127.
dc.identifier.urihttps://doi.org/10.3847/1538-4357/ad5be4
dc.identifier.urihttps://hdl.handle.net/10566/21252
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.subjectEarly-type galaxies
dc.subjectGalaxy circumnuclear disk
dc.subjectGalaxy nuclei
dc.subjectCircumnuclear Dust
dc.subjectEarly-type Galaxies
dc.titleCircumnuclear dust in luminous Early-type galaxies. i. sample properties and stellar luminosity models
dc.typeArticle

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