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_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Physics Department Collection
dc.relation.ispartofUMBC Faculty 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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