Results 21 to 30 of about 1,734 (149)

Silaj Mikro Florasının Birbirleri İle İlişkileri, Silaj Fermentasyonu ve Kalitesi Üzerine Etkileri

open access: yesKahramanmaraş Sütçü İmam Üniversitesi Doğa Bilimleri Dergisi, 2016
Ulkemizde silaj yapimi son yillarda giderek artan bir hizla yayginlasmaktadir. Silaj yapiminin teknigine uygun sekilde yapilmasi, ustun kaliteli silaj elde edilmesi icin bir on sarttir. Bununla birlikte silaj mikro florasi, bunlarin birbirleri ile iliskileri ve silo icerisindeki gelisimleri, silaj kalitesini belirleyen ana unsurlardan biridir.
Mustafa KIZILSIMSEK   +3 more
openaire   +2 more sources

Accurate age determinations of several nearby open clusters containing magnetic Ap stars

open access: yes, 2014
Aims: Our aim is to obtain ages that are as accurate as possible for the seven nearby open clusters alpha Per, Coma Ber, IC 2602, NGC 2232, NGC 2451A, NGC 2516, and NGC 6475, each of which contains at least one magnetic Ap or Bp star.
Landstreet, J. D., Silaj, J.
core   +1 more source

The Interaction Of Multiple Convection Zones In A-type Stars [PDF]

open access: yes, 2007
A-type stars have a complex internal structure with the possibility of multiple convection zones. If not sufficiently separated, such zones will interact through the convectively stable regions that lie between them.
Hurlburt   +19 more
core   +3 more sources

İkinci Ürün Koşullarında Mısır-Maş Fasulye Üretiminde Farklı Ekim Sistemlerinin Silaj Kalite ve Fermentasyonuna Etkisi

open access: yesISPEC Journal of Agricultural Sciences
Birlikte üretim, bir veya daha fazla benzer olmayan bitkinin aynı sıralarda veya farklı sıralarda birlikte yetiştirilmesi olarak tanımlanmaktadır. Bu çalışma, Kahramanmaraş ekolojik koşullarda mısır+maş fasulyesi bitkilerinin aynı sıra üzerinde farklı ...
Fatma AKBAY   +5 more
doaj   +1 more source

Warped disks during type II outbursts in Be/X-ray binaries: evidence from optical polarimetry

open access: yes, 2018
Current models that explain giant (type II) X-ray outbursts in Be/X-ray binaries (BeXB), are based on the idea of highly distorted disks. They are believed to occur when a misaligned and warped disk becomes eccentric, allowing the neutron star to capture
Blinov, D., Reig, P.
core   +1 more source

Inhibition of thermohaline mixing by a magnetic field in Ap star descendants: Implications for the Galactic evolution of 3He

open access: yes, 2007
To reconcile the measurements of 3He/H in Galactic HII regions with high values of 3He in a couple of planetary nebulae, we propose that thermohaline mixing is inhibited by a fossil magnetic field in red giant stars that are descendants of Ap stars.
Bagnulo   +41 more
core   +2 more sources

Mısır Silajının Fermantasyon, Aerobik Stabilite Özellikleri Üzerine Aktifleştirilen Lactobacillus buchneri ve Üre İlavesinin Etkileri

open access: yesTurkish Journal of Agriculture: Food Science and Technology, 2023
Bu çalışma, silolama öncesi aktifleştirilen Lactobacillus buchneri (NCIMB 40788 ˗ CNCM I-4323; Lalsil AS, Lallemand Inc., Canada) inokulantının mısır silajına üre ile ilavesinin fermantasyon ve aerobik stabilite üzerine etkilerini belirlemek amacıyla ...
Caner Bağcık   +2 more
doaj   +1 more source

A Pre-Gaia Census of Nearby Stellar Groups

open access: yes, 2015
The nearest, youngest groups of stars to the Sun provide important samples of age-dated stars for studying circumstellar disk evolution, imaged exoplanets, and brown dwarfs.
Mamajek, Eric E.
core   +1 more source

Magnetic Field Generation in Stars [PDF]

open access: yes, 2015
Enormous progress has been made on observing stellar magnetism in stars from the main sequence through to compact objects. Recent data have thrown into sharper relief the vexed question of the origin of stellar magnetic fields, which remains one of the ...
A. Beresnyak   +242 more
core   +2 more sources

The Oxford handbook of publishing / edited by Angus Phillips and Michael Bhaskar

open access: yesVjesnik Bibliotekara Hrvatske, 2021
The Oxford handbook of publishing / edited by Angus Phillips and Michael Bhaskar. Oxford University Press, 2019. 480 str.
Kristina Silaj
doaj  

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