dc.contributor.author |
Marleau, Gabriel-Dominique |
|
dc.date.accessioned |
2022-03-24T15:14:35Z |
|
dc.date.available |
2022-03-24T15:14:35Z |
|
dc.date.issued |
2021 |
|
dc.identifier.issn |
2041-8213 |
|
dc.identifier.uri |
http://hdl.handle.net/10900/125567 |
|
dc.language.iso |
en |
en |
dc.publisher |
Iop Publishing Ltd |
de_DE |
dc.relation.uri |
http://dx.doi.org/10.3847/2041-8213/ac19bd |
|
dc.subject.ddc |
520 |
de_DE |
dc.subject.ddc |
530 |
de_DE |
dc.title |
Comparison of Planetary H alpha-emission Models: A New Correlation with Accretion Luminosity |
de_DE |
dc.type |
Article |
de_DE |
utue.quellen.id |
20211125174918_01169 |
|
utue.personen.roh |
Aoyama, Yuhiko |
|
utue.personen.roh |
Marleau, Gabriel-Dominique |
|
utue.personen.roh |
Ikoma, Masahiro |
|
utue.personen.roh |
Mordasini, Christoph |
|
dcterms.isPartOf.ZSTitelID |
Astrophysical Journal Letters |
de_DE |
dcterms.isPartOf.ZS-Issue |
Article L30 |
de_DE |
dcterms.isPartOf.ZS-Volume |
917 |
de_DE |
utue.fakultaet |
07 Mathematisch-Naturwissenschaftliche Fakultät |
|