Cold dust but warm gas in the unusual elliptical galaxy NGC 4125

Wilson, C. D., Cridland, A., Foyle, K., Parkin, T. J., Cooper, E. Mentuch, Roussel, H., Sauvage, M., Smith, Matthew ORCID: https://orcid.org/0000-0002-3532-6970, Baes, M., Bendo, G., Boquien, M., Boselli, A., Ciesla, L., Clements, D. L., Cooray, A., De Looze, I., Galametz, M., Gear, W., Lebouteiller, V., Madden, S., Pereira-Santaella, M. and Rémy-Ruyer, A. 2013. Cold dust but warm gas in the unusual elliptical galaxy NGC 4125. Astrophysical Journal Letters 776 (2) , L30. 10.1088/2041-8205/776/2/L30

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Abstract

Data from the Herschel Space Observatory have revealed an unusual elliptical galaxy, NGC 4125, which has strong and extended submillimeter emission from cold dust but only very strict upper limits to its CO and H I emission. Depending on the dust emissivity, the total dust mass is 2-5 × 106 M ☉. While the neutral gas-to-dust mass ratio is extremely low (<12-30), including the ionized gas traced by [C II] emission raises this limit to <39-100. The dust emission follows a similar r 1/4 profile to the stellar light and the dust to stellar mass ratio is toward the high end of what is found in nearby elliptical galaxies. We suggest that NGC 4125 is currently in an unusual phase where evolved stars produced in a merger-triggered burst of star formation are pumping large amounts of gas and dust into the interstellar medium. In this scenario, the low neutral gas-to-dust mass ratio is explained by the gas being heated to temperatures ≥104 K faster than the dust is evaporated. If galaxies like NGC 4125, where the far-infrared emission does not trace neutral gas in the usual manner, are common at higher redshift, this could have significant implications for our understanding of high redshift galaxies and galaxy evolution.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	American Astronomical Society
ISSN:	2041-8205
Date of First Compliant Deposit:	6 December 2017
Date of Acceptance:	20 September 2013
Last Modified:	05 May 2023 13:33
URI:	https://orca.cardiff.ac.uk/id/eprint/107368

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