Hot Gas Outflow Properties of the Starburst Galaxy NGC 4945

dc.contributor.authorBarrera, Natalia Porraz
dc.contributor.authorLopez, Sebastian
dc.contributor.authorLopez, Laura A.
dc.contributor.authorFoord, Adi
dc.contributor.authorNguyen, Dustin D.
dc.contributor.authorThompson, Todd A.
dc.contributor.authorBolatto, Alberto D.
dc.date.accessioned2024-01-12T13:17:11Z
dc.date.available2024-01-12T13:17:11Z
dc.date.issued2023-12-13
dc.description.abstractWe analyze 330 ks of {\it Chandra} X-ray imaging and spectra of the nearby, edge-on starburst and Seyfert Type 2 galaxy NGC~4945 to measure the hot gas properties along the galactic outflows. We extract and model spectra from 15 regions extending from −0.55 kpc to +0.85 kpc above and below the galactic disk to determine the best-fit parameters and metal abundances. We find that the hot gas temperatures and number densities peak in the central regions and decrease along the outflows. These profiles are inconsistent with a spherical, adiabatically-expanding wind model, suggesting the need to include mass loading and/or a non-spherical outflow geometry. We estimate the mass outflow rate of the hot wind to be 2.1M⊙ yr⁻¹. Emission from charge exchange is detected in the northern outflow, and we estimate it contributes 12\% to the emitted, broad-band (0.5−7~keV) X-ray flux.
dc.description.sponsorshipNPB, SL, and LAL were supported by NASA’s Astrophysics Data Analysis Program under grant number 80NSSC22K0496 and by the Heising-Simons Foundation through grant number 2022-3533. LAL also acknowledges the support of the Simons Foundation. We thank the OSU Galaxy/ISM Meeting for useful discussions. DDN acknowledges funding from NASA 21-ASTRO21- 0174.
dc.description.urihttps://arxiv.org/abs/2312.08444
dc.format.extent10 pages
dc.genrejournal articles
dc.genrepreprints
dc.identifier.urihttps://doi.org/10.48550/arXiv.2312.08444
dc.identifier.urihttp://hdl.handle.net/11603/31290
dc.language.isoen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Faculty Collection
dc.relation.ispartofUMBC Physics Department Collection
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.titleHot Gas Outflow Properties of the Starburst Galaxy NGC 4945
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0002-1616-1701

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