The dust-continuum size of TNG50 galaxies at z = 1-5: a comparison with the distribution of stellar light, stars, dust, and H2
We present predictions for the extent of the dust-continuum emission of main-sequence galaxies drawn from the TNG50 simulation in the range z = 1-5. We couple the radiative transfer code SKIRT to the output of the TNG50 simulation and measure the dust-continuum half-light radius of the modelled gala...
Gespeichert in:
| Hauptverfasser: | , , , , , , , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2022
|
| In: |
Monthly notices of the Royal Astronomical Society
Year: 2022, Jahrgang: 510, Heft: 3, Pages: 3321-3334 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stab3312 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stab3312
|
| Verfasserangaben: | Gergö Popping, Annalisa Pillepich, Gabriela Calistro Rivera, Sebastian Schulz, Lars Hernquist, Melanie Kaasinen, Federico Marinacci, Dylan Nelson and Mark Vogelsberger |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1799522180 | ||
| 003 | DE-627 | ||
| 005 | 20240821122959.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 220413s2022 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1093/mnras/stab3312 |2 doi | |
| 035 | |a (DE-627)1799522180 | ||
| 035 | |a (DE-599)KXP1799522180 | ||
| 035 | |a (OCoLC)1341458997 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Popping, Gergö |e VerfasserIn |0 (DE-588)1255776161 |0 (DE-627)179993103X |4 aut | |
| 245 | 1 | 4 | |a The dust-continuum size of TNG50 galaxies at z = 1-5 |b a comparison with the distribution of stellar light, stars, dust, and H2 |c Gergö Popping, Annalisa Pillepich, Gabriela Calistro Rivera, Sebastian Schulz, Lars Hernquist, Melanie Kaasinen, Federico Marinacci, Dylan Nelson and Mark Vogelsberger |
| 264 | 1 | |c 2022 | |
| 300 | |a 14 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Advance access publication 2021 November 18 | ||
| 500 | |a Gesehen am 21.04.2022 | ||
| 520 | |a We present predictions for the extent of the dust-continuum emission of main-sequence galaxies drawn from the TNG50 simulation in the range z = 1-5. We couple the radiative transfer code SKIRT to the output of the TNG50 simulation and measure the dust-continuum half-light radius of the modelled galaxies, assuming a Milky Way dust type and a metallicity-dependent dust-to-metal ratio. The dust-continuum half-light radius at observed-frame 850 $\m |m is up to ∼75 per cent larger than the stellar half-mass radius, but significantly more compact than the observed-frame 1.6 $\m |m (roughly corresponding to H band) half-light radius, particularly towards high redshifts: the compactness compared to the 1.6 $\m |m emission increases with redshift. This is driven by obscuration of stellar light from the galaxy centres, which increases the apparent extent of 1.6 $\m |m disc sizes relative to that at 850 $\mu$m. The difference in relative extents increases with redshift because the observed-frame 1.6 $\m |m emission stems from ever shorter wavelength stellar emission. These results suggest that the compact dust-continuum emission observed in z > 1 galaxies is not (necessarily) evidence of the build-up of a dense central stellar component. We find that the dust-continuum half-light radius closely follows the radius containing half the star formation and half the dust mass in galaxies and is ∼80 per cent of the radius containing half the H2 mass. The presented results are a common feature of main-sequence galaxies. | ||
| 700 | 1 | |a Pillepich, Annalisa |e VerfasserIn |0 (DE-588)1151829854 |0 (DE-627)1012339327 |0 (DE-576)423800841 |4 aut | |
| 700 | 1 | |a Calistro Rivera, Gabriela |e VerfasserIn |4 aut | |
| 700 | 1 | |a Schulz, Sebastian |e VerfasserIn |4 aut | |
| 700 | 1 | |a Hernquist, Lars |d 1954- |e VerfasserIn |0 (DE-588)1264244401 |0 (DE-627)1813088241 |4 aut | |
| 700 | 1 | |a Kaasinen, Melanie |d 1994- |e VerfasserIn |0 (DE-588)1198901357 |0 (DE-627)1681083140 |4 aut | |
| 700 | 1 | |a Marinacci, Federico |e VerfasserIn |0 (DE-588)1054438684 |0 (DE-627)79152194X |0 (DE-576)410132837 |4 aut | |
| 700 | 1 | |a Nelson, Dylan |e VerfasserIn |0 (DE-588)115182805X |0 (DE-627)101233600X |0 (DE-576)42382581X |4 aut | |
| 700 | 1 | |a Vogelsberger, Mark |d 1978- |e VerfasserIn |0 (DE-588)133437698 |0 (DE-627)546058434 |0 (DE-576)299848299 |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |a Royal Astronomical Society |t Monthly notices of the Royal Astronomical Society |d Oxford : Oxford Univ. Press, 1827 |g 510(2022), 3, Seite 3321-3334 |h Online-Ressource |w (DE-627)314059164 |w (DE-600)2016084-7 |w (DE-576)090955420 |x 1365-2966 |7 nnas |
| 773 | 1 | 8 | |g volume:510 |g year:2022 |g number:3 |g pages:3321-3334 |g extent:14 |a The dust-continuum size of TNG50 galaxies at z = 1-5 a comparison with the distribution of stellar light, stars, dust, and H2 |
| 856 | 4 | 0 | |u https://doi.org/10.1093/mnras/stab3312 |x Verlag |x Resolving-System |z lizenzpflichtig |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20220413 | ||
| 993 | |a Article | ||
| 994 | |a 2022 | ||
| 998 | |g 115182805X |a Nelson, Dylan |m 115182805X:Nelson, Dylan |d 700000 |d 714000 |d 714200 |d 700000 |d 728500 |e 700000PN115182805X |e 714000PN115182805X |e 714200PN115182805X |e 700000PN115182805X |e 728500PN115182805X |k 0/700000/ |k 1/700000/714000/ |k 2/700000/714000/714200/ |k 0/700000/ |k 1/700000/728500/ |p 8 | ||
| 998 | |g 1198901357 |a Kaasinen, Melanie |m 1198901357:Kaasinen, Melanie |d 700000 |d 714000 |d 714200 |e 700000PK1198901357 |e 714000PK1198901357 |e 714200PK1198901357 |k 0/700000/ |k 1/700000/714000/ |k 2/700000/714000/714200/ |p 6 | ||
| 998 | |g 1151829854 |a Pillepich, Annalisa |m 1151829854:Pillepich, Annalisa |d 130000 |d 700000 |d 728500 |e 130000PP1151829854 |e 700000PP1151829854 |e 728500PP1151829854 |k 0/130000/ |k 0/700000/ |k 1/700000/728500/ |p 2 | ||
| 999 | |a KXP-PPN1799522180 |e 4117265377 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"name":{"displayForm":["Gergö Popping, Annalisa Pillepich, Gabriela Calistro Rivera, Sebastian Schulz, Lars Hernquist, Melanie Kaasinen, Federico Marinacci, Dylan Nelson and Mark Vogelsberger"]},"origin":[{"dateIssuedDisp":"2022","dateIssuedKey":"2022"}],"language":["eng"],"note":["Advance access publication 2021 November 18","Gesehen am 21.04.2022"],"recId":"1799522180","type":{"bibl":"article-journal","media":"Online-Ressource"},"title":[{"title_sort":"dust-continuum size of TNG50 galaxies at z = 1-5","title":"The dust-continuum size of TNG50 galaxies at z = 1-5","subtitle":"a comparison with the distribution of stellar light, stars, dust, and H2"}],"relHost":[{"part":{"pages":"3321-3334","issue":"3","extent":"14","volume":"510","year":"2022","text":"510(2022), 3, Seite 3321-3334"},"disp":"Royal Astronomical SocietyMonthly notices of the Royal Astronomical Society","corporate":[{"display":"Royal Astronomical Society","role":"aut"}],"id":{"eki":["314059164"],"doi":["10.1111/(ISSN)1365-2966"],"issn":["1365-2966"],"zdb":["2016084-7"]},"type":{"bibl":"periodical","media":"Online-Ressource"},"physDesc":[{"extent":"Online-Ressource"}],"title":[{"title":"Monthly notices of the Royal Astronomical Society","title_sort":"Monthly notices of the Royal Astronomical Society"}],"note":["Gesehen am 15.01.2018"],"recId":"314059164","language":["eng"],"origin":[{"publisher":"Oxford Univ. Press ; Blackwell ; Wiley-Blackwell","dateIssuedDisp":"1827-","dateIssuedKey":"1827","publisherPlace":"Oxford ; Oxford [u.a.] ; Oxford [u.a.]"}],"pubHistory":["1.1827 -"]}],"physDesc":[{"extent":"14 S."}],"id":{"doi":["10.1093/mnras/stab3312"],"eki":["1799522180"]},"person":[{"display":"Popping, Gergö","family":"Popping","given":"Gergö","role":"aut"},{"given":"Annalisa","role":"aut","display":"Pillepich, Annalisa","family":"Pillepich"},{"display":"Calistro Rivera, Gabriela","family":"Calistro Rivera","given":"Gabriela","role":"aut"},{"family":"Schulz","display":"Schulz, Sebastian","role":"aut","given":"Sebastian"},{"display":"Hernquist, Lars","family":"Hernquist","given":"Lars","role":"aut"},{"family":"Kaasinen","display":"Kaasinen, Melanie","role":"aut","given":"Melanie"},{"display":"Marinacci, Federico","family":"Marinacci","given":"Federico","role":"aut"},{"display":"Nelson, Dylan","family":"Nelson","given":"Dylan","role":"aut"},{"role":"aut","given":"Mark","family":"Vogelsberger","display":"Vogelsberger, Mark"}]} | ||
| SRT | |a POPPINGGERDUSTCONTIN2022 | ||