http://ir.sinica.edu.tw/handle/201000000A/87464
DC Field | Value | Language |
---|---|---|
dc.contributor | 天文及天文物理研究所 | - |
dc.contributor.author | Relaño, M | - |
dc.contributor.author | De Looze, I | - |
dc.contributor.author | Saintonge, A | - |
dc.contributor.author | Hou, K-C | - |
dc.contributor.author | Romano, L E C | - |
dc.contributor.author | Nagamine, K | - |
dc.contributor.author | Hirashita, H | - |
dc.contributor.author | Aoyama, S | - |
dc.contributor.author | Lamperti, I | - |
dc.contributor.author | Lisenfeld, U | - |
dc.contributor.author | Smith, M W L | - |
dc.contributor.author | Chastenet, J | - |
dc.contributor.author | Xiao, T | - |
dc.contributor.author | Gao, Y | - |
dc.contributor.author | Sargent, M | - |
dc.contributor.author | van der Giessen, S A | - |
dc.date.accessioned | 2024-01-16T02:29:50Z | - |
dc.date.available | 2024-01-16T02:29:50Z | - |
dc.date.issued | 2022-08-18 | - |
dc.identifier.issn | http://gateway.isiknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Drexel&SrcApp=hagerty_opac&KeyRecord=0035-8711&DestApp=JCR&RQ=IF_CAT_BOXPLOT | - |
dc.identifier.uri | http://ir.sinica.edu.tw/handle/201000000A/87464 | - |
dc.description.sponsorship | 天文及天文物理研究所 | - |
dc.language.iso | en | - |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society 515(4), 5306-5334 | - |
dc.title | Dust grain size evolution in local galaxies: a comparison between observations and simulations | - |
dc.type | journal article | - |
dc.identifier.url | http://dx.doi.org/10.1093/mnras/stac2108 | - |
dc.description.note | 已出版;[SCI];有審查制度;具代表性 | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | none | - |
item.openairetype | journal article | - |
item.fulltext | no fulltext | - |
item.openairecristype | http://purl.org/coar/resource_type/c_6501 | - |
crisitem.author.dept | Institute of Astronomy and Astrophysics | - |
crisitem.author.parentorg | Division of Mathematics and Physical Sciences | - |
Appears in Collections: | 天文及天文物理研究所 |
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