Zobrazeno 1 - 10
of 42
pro vyhledávání: '"David A. Strickland"'
Publikováno v:
PhytoFrontiers, Vol 4, Iss 2, Pp 141-149 (2024)
Scarf skin is a fruit finish disorder of apple that leads to reduced grade quality and rejected crop loads. Although not established as a disorder specific to certain cultivars, the manifestation of the disorder is more apparent on red-skinned cultiv
Externí odkaz:
https://doaj.org/article/58fe7d4bbf54428f9e4cb5e1de16e05b
Publikováno v:
Plant Disease. 107:1425-1432
In the absence of durable host resistance among commercial cultivars, chemical management continues to be an essential component of disease control in apple production. Apple powdery mildew, caused by the ascomycete Podosphaera leucotricha, is largel
The postharvest fruit pathogenPaecilomyces niveusproduces ascospores that can survive some pasteurization temperatures, spoil fruit products, and contaminate them with patulin, an FDA-regulated mycotoxin. PreventingP. niveusfrom entering food systems
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e61a67cb41b307b56ad808e1bbc6c86e
https://doi.org/10.1101/2023.02.18.529073
https://doi.org/10.1101/2023.02.18.529073
Publikováno v:
Plant Disease. 107:216
In late July and August 2015, foliar disease was observed in three hop (Humulus lupulus; unknown cultivars) yards in Ontario, Otsego, and Putnam counties, New York (NY). Disease incidence ranged between 70 and 90% of plants, and up to 25% of the leav
Publikováno v:
Plant disease. 106(4)
Powdery mildew, caused by the ascomycete
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 362:626-648
In this paper we present high-resolution hydrodynamical models of warm ionized clouds embedded in a superwind, and compare the OVI and soft X-ray properties to the existing observational data. These models include thermal conduction, which we show pl
Publikováno v:
The Astrophysical Journal. 628:113-128
We found several extranuclear (r >~ 3") X-ray nebulae within 40" (6.3 kpc at 32.5 Mpc) of the nucleus of the Seyfert galaxy NGC 2992. The net X-ray luminosity from the extranuclear sources is ~2-3 E39 erg/s (0.3-8.0 keV). The X-ray core itself (r
Publikováno v:
The Astrophysical Journal. 628:187-204
We have analyzed observations with the Chandra X-ray Observatory of the diffuse emission by hot gas in 7 dwarf starburst galaxies, 6 edge-on starburst galaxies, and 9 Ultra Luminous Infrared Galaxies. These systems cover ranges of \~ 10^4 in X-ray lu
Publikováno v:
The Astrophysical Journal. 592:782-803
We present initial results from a Chandra survey of a complete sample of the eight nearest (z ≤ 0.04) ultraluminous IR galaxies (ULIRGs) and also include the IR-luminous galaxy NGC 6240 for comparison. In this paper we use the hard X-rays (2-8 keV)
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 342:690-708
We present CHANDRA X-ray data of the nearby Magellanic Irregular dwarf starburst galaxy NGC4449. Contributions to the X-ray emission come from discrete point sources and extended diffuse emission. The extended emission has a complex morphology with a