Results 171 to 180 of about 3,506 (220)
Screening of lentil genotypes against stemphylium blight disease and molecular identification of causal organism. [PDF]
Aktar-Uz-Zaman M +8 more
europepmc +1 more source
Patients potentially in need for palliative care in Germany-A regional small-area estimation based on death registry data. [PDF]
Gesell D +4 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Open market share repurchases and the free cash flow hypothesis G35
Economics Letters, 1995zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Nikos Vafeas, O Maurice Joy
exaly +3 more sources
The BeppoSAX observation of the Seyfert 1.9 galaxy ESO103-G35
We present results from BeppoSAX observations of the Seyfert 1.9 Galaxy ESO103-G35. The LEGS, MECS and PDS spectra (0.1-200 keV) allows us to better understand the nature of this object. We find that the spectra can be described by a powerlaw with a photon index typical of a Seyfert 1 with a cutoff at high energies and a large absorption column density,
Antonelli LA +5 more
openaire +2 more sources
G35 Crohns disease: Initial treatment and outcomes at 12 months: Abstract G35 Table 1
Archives of Disease in Childhood, 2016Introduction Exclusive enteral nutrition (EEN) is the primary therapy for induction of remission and growth restoration in newly diagnosed children with Crohns Disease (CD). Patients who failed to go into clinical remission were offered steroids with partial enteral nutrition (PEN) alongside diet or steroids alone.
J Gavin +4 more
openaire +1 more source
‘G35’ Sainfoin (Onobrychis viciifolia Scop.)
New Zealand Journal of Agricultural Research, 2005(2005). ‘G35’ Sainfoin (Onobrychis viciifolia Scop.) New Zealand Journal of Agricultural Research: Vol. 48, No. 1, pp. 127-128.
W. Rumball, R. B. Claydon
openaire +1 more source
1991
The DQ G35-26 is spectroscopically analyzed and the results discussed in the context of dredge-up of carbon and the accretion of hydrogen. The best fit is T eff=13,000K with firm limits between 11,000K and 14,000K, log(g) between 9.0 and 9.5. The hydrogen abundance is close to 1% by number and the carbon abundance close to 3%.
Peter Thejll +2 more
openaire +1 more source
The DQ G35-26 is spectroscopically analyzed and the results discussed in the context of dredge-up of carbon and the accretion of hydrogen. The best fit is T eff=13,000K with firm limits between 11,000K and 14,000K, log(g) between 9.0 and 9.5. The hydrogen abundance is close to 1% by number and the carbon abundance close to 3%.
Peter Thejll +2 more
openaire +1 more source

