I agree that this site is using cookies. You can find further informations
here
.
X
Login
Merkliste (
0
)
Home
About us
Home About us
Our history
Profile
Press & public relations
Friends
The library in figures
Exhibitions
Projects
Training, internships, careers
Films
Services & Information
Home Services & Information
Lending and interlibrary loans
Returns and renewals
Training and library tours
My Account
Library cards
New to the library?
Download Information
Opening hours
Learning spaces
PC, WLAN, copy, scan and print
Catalogs and collections
Home Catalogs and Collections
Rare books and manuscripts
Digital collections
Subject Areas
Our sites
Home Our sites
Central Library
Law Library (Juridicum)
BB Business and Economics (BB11)
BB Physics and Electrical Engineering
TB Engineering and Social Sciences
TB Economics and Nautical Sciences
TB Music
TB Art & Design
TB Bremerhaven
Contact the library
Home Contact the library
Staff Directory
Open access & publishing
Home Open access & publishing
Reference management: Citavi & RefWorks
Publishing documents
Open Access in Bremen
zur Desktop-Version
Toggle navigation
Merkliste
1 Ergebnisse
1
The gas-phase metallicities of star-forming galaxies in ape..:
D'Eugenio, Francesco
;
Colless, Matthew
;
Groves, Brent
..
Monthly Notices of the Royal Astronomical Society. 479 (2018) 2 - p. 1807-1821 , 2018
Link:
https://doi.org/10.1093/mnras/sty1424
RT Journal T1
The gas-phase metallicities of star-forming galaxies in aperture-matched SDSS samples follow potential rather than mass or average surface density
UL https://suche.suub.uni-bremen.de/peid=cr-10.1093_mnras_sty1424&Exemplar=1&LAN=DE A1 D'Eugenio, Francesco A1 Colless, Matthew A1 Groves, Brent A1 Bian, Fuyan A1 Barone, Tania M PB Oxford University Press (OUP) YR 2018 SN 0035-8711 SN 1365-2966 JF Monthly Notices of the Royal Astronomical Society VO 479 IS 2 SP 1807 OP 1821 LK http://dx.doi.org/https://doi.org/10.1093/mnras/sty1424 DO https://doi.org/10.1093/mnras/sty1424 SF ELIB - SuUB Bremen
Export
RefWorks (nur Desktop-Version!)
Flow
(Zuerst in
Flow
einloggen, dann importieren)