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Sökning: onr:"swepub:oai:DiVA.org:su-195956" > Studying the ISM at...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00005543naa a2200517 4500
001oai:DiVA.org:su-195956
003SwePub
008210830s2021 | |||||||||||000 ||eng|
0247 a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1959562 URI
0247 a https://doi.org/10.1051/0004-6361/2020394022 DOI
040 a (SwePub)su
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
1001 a Della Bruna, Lorenzau Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)lode4798
2451 0a Studying the ISM at similar to 10 pc scale in NGC 7793 with MUSE :b II. Constraints on the oxygen abundance and ionising radiation escape
264 c 2021-06-15
264 1b EDP Sciences,c 2021
338 a print2 rdacarrier
520 a Context. Feedback from massive stars a ffects the interstellar medium (ISM) from the immediate surroundings of the stars (parsec scales) to galactic (kiloparsec) scales. High-spatial resolution studies of H ii regions are critical to investigate how this mechanism operates.Aims. We study the ionised ISM in NGC7793 with the MUSE instrument at ESO Very Large Telescope (VLT), over a field of view (FoV) of similar to 2 kpc2 and at a spatial resolution of similar to 10 pc. The aim is to link the physical conditions of the ionised gas (reddening, ionisation status, abundance measurements) within the spatially resolved H ii regions to the properties of the stellar populations producing Lyman continuum photons.Methods. The analysis of the MUSE dataset, which provides a map of the ionised gas and a census of Wolf Rayet stars, is complemented with a sample of young star clusters (YSCs) and O star candidates observed with the Hubble Space Telescope (HST) and of giant molecular clouds traced in CO(2-1) emission with the Atacama Large Millimeter /submillimeter Array (ALMA). We estimated the oxygen abundance using a temperature-independent strong-line method. We determined the observed total amount of ionising photons ( Q(H0)) from the extinction corrected H ff luminosity. This estimate was then compared to the expected Q(H0) obtained by summing the contributions of YSCs and massive stars. The ratio of the two values gives an estimate for the escape fraction ( fesc) of photons in the region of interest. We used the [S ii] /[O iii] ratio as a proxy for the optical depth of the gas and classified H ii regions into ionisation bounded, or as featuring channels of optically thin gas. We compared the resulting ionisation structure with the computed fesc. We also investigated the dependence of fesc on the age spanned by the stellar population in each region.Results. We find a median oxygen abundance of 12 + log (O =H) similar to 8 :37, with a scatter of 0.25 dex, which is in agreement with previous estimates for our target. We furthermore observe that the abundance map of H ii regions is rich in substructures, surrounding clusters and massive stars, although clear degeneracies with photoionisation are also observed. From the population synthesis analysis, we find that YSCs located in H ii regions have a higher probability of being younger and less massive as well as of emitting a higher number of ionising photons than clusters in the rest of the field. Overall, we find fesc;H ii = 0:67+0:08 0:12 for the population of H ii regions. We also conclude that the sources of ionisation observed within the FoV are more than su fficient to explain the amount of di ffuse ionised gas (DIG) observed in this region of the galaxy. We do not observe a systematic trend between the visual appearance of H ii regions and fesc, pointing to the e ffect of 3D geometry in the small sample probed.
650 7a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng
653 a galaxies: ISM
653 a HII regions
653 a galaxies: individual: NGC 7793
653 a ISM: structure
653 a ISM: general
7001 a Adamo, Angelau Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)anad2127
7001 a Lee, Janice C.4 aut
7001 a Smith, Linda J.4 aut
7001 a Krumholz, Mark4 aut
7001 a Bik, Arjanu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)abik
7001 a Calzetti, Daniela4 aut
7001 a Fox, Anneu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut
7001 a Fumagalli, Michele4 aut
7001 a Grasha, Kathryn4 aut
7001 a Messa, Matteou Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC),Université de Genève, Switzerland4 aut0 (Swepub:su)mame4466
7001 a Östlin, Göranu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)ostlin
7001 a Walterbos, Rene4 aut
7001 a Wofford, Aida4 aut
7102 a Stockholms universitetb Institutionen för astronomi4 org
7730 t Astronomy and Astrophysicsd : EDP Sciencesg 650q 650x 0004-6361x 1432-0746
8564 u https://authors.library.caltech.edu/109858/1/aa39402-20.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-195956
8564 8u https://doi.org/10.1051/0004-6361/202039402

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