dc.contributor.author |
Suchy, Slawomir |
|
dc.date.accessioned |
2013-07-18T08:12:58Z |
|
dc.date.available |
2013-07-18T08:12:58Z |
|
dc.date.issued |
2013 |
|
dc.identifier.issn |
0004-637X |
|
dc.identifier.uri |
http://hdl.handle.net/10900/36063 |
|
dc.language.iso |
en |
de_DE |
dc.publisher |
Iop Publishing Ltd |
de_DE |
dc.relation.uri |
http://dx.doi.org/10.1088/0004-637X/762/1/61 |
|
dc.rights |
info:eu-repo/semantics/closedAccess |
|
dc.subject.ddc |
520 |
de_DE |
dc.subject.ddc |
530 |
de_DE |
dc.title |
THE Be/X-RAY BINARY SWIFT J1626.6-5156 AS A VARIABLE CYCLOTRON LINE SOURCE |
de_DE |
dc.type |
Article |
de_DE |
utue.quellen.id |
20130315161744_00350 |
de_DE |
utue.personen.roh |
DeCesar, Megan E. |
|
utue.personen.roh |
Boyd, Patricia T. |
|
utue.personen.roh |
Pottschmidt, Katja |
|
utue.personen.roh |
Wilms, Joern |
|
utue.personen.roh |
Suchy, Slawomir |
|
utue.personen.roh |
Miller, M. Coleman |
|
dcterms.isPartOf.ZSTitelID |
Astrophysical Journal |
de_DE |
dcterms.isPartOf.ZS-Issue |
Article 61 |
de_DE |
dcterms.isPartOf.ZS-Volume |
762 |
de_DE |
utue.fakultaet |
07 Mathematisch-Naturwissenschaftliche Fakultät |
de_DE |