Brightness variations caused by surface magnetic fields in pre-main-sequence stars
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
1984
|
| In: |
The astrophysical journal
Year: 1984, Jahrgang: 278, Pages: 689-694 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://adsabs.harvard.edu/full/1984ApJ...278..689A
|
| Verfasserangaben: | I. Appenzeller, D.S.P. Dearborn |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1523470607 | ||
| 003 | DE-627 | ||
| 005 | 20220812130231.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 151217s1984 xx |||||o 00| ||eng c | ||
| 035 | |a (DE-627)1523470607 | ||
| 035 | |a (DE-576)453470602 | ||
| 035 | |a (DE-599)BSZ453470602 | ||
| 035 | |a (OCoLC)1340894997 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Appenzeller, Immo |d 1940- |e VerfasserIn |0 (DE-588)131650092 |0 (DE-627)512043353 |0 (DE-576)16009349X |4 aut | |
| 245 | 1 | 0 | |a Brightness variations caused by surface magnetic fields in pre-main-sequence stars |c I. Appenzeller, D.S.P. Dearborn |
| 264 | 1 | |c 1984 | |
| 300 | |a 6 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 700 | 1 | |a Dearborn, David S. P. |d 1949- |e VerfasserIn |0 (DE-588)1033755583 |0 (DE-627)742469417 |0 (DE-576)175888922 |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t The astrophysical journal |d Chicago, Ill. [u.a.] : Univ., 1895 |g 278(1984), Seite 689-694 |h Online-Ressource |w (DE-627)502174293 |w (DE-600)2207648-7 |w (DE-576)281290024 |7 nnas |a Brightness variations caused by surface magnetic fields in pre-main-sequence stars |
| 773 | 1 | 8 | |g volume:278 |g year:1984 |g pages:689-694 |g extent:6 |a Brightness variations caused by surface magnetic fields in pre-main-sequence stars |
| 856 | 4 | 0 | |u http://adsabs.harvard.edu/full/1984ApJ...278..689A |x Verlag |x Resolving-System |z kostenfrei |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20151217 | ||
| 993 | |a Article | ||
| 994 | |a 1984 | ||
| 998 | |g 131650092 |a Appenzeller, Immo |m 131650092:Appenzeller, Immo |d 700000 |d 714000 |d 714300 |e 700000PA131650092 |e 714000PA131650092 |e 714300PA131650092 |k 0/700000/ |k 1/700000/714000/ |k 2/700000/714000/714300/ |p 1 |x j | ||
| 999 | |a KXP-PPN1523470607 |e 2876210398 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"name":{"displayForm":["I. Appenzeller, D.S.P. Dearborn"]},"person":[{"family":"Appenzeller","given":"Immo","roleDisplay":"VerfasserIn","display":"Appenzeller, Immo","role":"aut"},{"role":"aut","display":"Dearborn, David S. P.","roleDisplay":"VerfasserIn","given":"David S. P.","family":"Dearborn"}],"origin":[{"dateIssuedKey":"1984","dateIssuedDisp":"1984"}],"title":[{"title":"Brightness variations caused by surface magnetic fields in pre-main-sequence stars","title_sort":"Brightness variations caused by surface magnetic fields in pre-main-sequence stars"}],"id":{"eki":["1523470607"]},"physDesc":[{"extent":"6 S."}],"type":{"bibl":"article-journal","media":"Online-Ressource"},"language":["eng"],"relHost":[{"origin":[{"publisherPlace":"Chicago, Ill. [u.a.]","publisher":"Univ.","dateIssuedKey":"1895","dateIssuedDisp":"1895-1996"}],"id":{"zdb":["2207648-7"],"eki":["502174293"]},"physDesc":[{"extent":"Online-Ressource"}],"title":[{"title_sort":"astrophysical journal","title":"The astrophysical journal"}],"pubHistory":["1.1895 - 473.1996"],"part":{"pages":"689-694","year":"1984","extent":"6","volume":"278","text":"278(1984), Seite 689-694"},"type":{"media":"Online-Ressource","bibl":"periodical"},"note":["Gesehen am 15.02.2021"],"disp":"Brightness variations caused by surface magnetic fields in pre-main-sequence starsThe astrophysical journal","recId":"502174293","language":["eng"]}],"recId":"1523470607"} | ||
| SRT | |a APPENZELLEBRIGHTNESS1984 | ||