Skip to search formSkip to main contentSkip to account menu

Ramularia collo-cygni

Known as: Ophiocladium hordei, Ovularia hordei 
National Institutes of Health

Papers overview

Semantic Scholar uses AI to extract papers important to this topic.
2016
2016
FERMI GBM OBSERVATIONS OF V404 CYG DURING ITS 2015 OUTBURST
V404 Cygni was discovered in 1989 by the Ginga X-ray satellite during its only previously observed X-ray outburst and soon after… 
2015
2015
MILDEW LOCUS O Mutation Does Not Affect Resistance to Grain Infections with Fusarium spp. and Ramularia collo-cygni.
MILDEW LOCUS O defines a major susceptibility gene for powdery mildew, and recessive mlo resistance alleles are widely used in… 
2015
2015
Long-Term Multicolour Photometry of the Young Stellar Objects FHO 26, FHO 27, FHO 28, FHO 29, and V1929 Cygni
Abstract Results from long-term multicolour optical photometric observations of the pre-main-sequence stars FHO 26, FHO 27, FHO… 
2013
2013
Fermi Discovers a New Population of Gamma-ray Novae
Novae had not been widely considered as high-energy (>100 MeV) gamma-ray sources before the launch of the Fermi Large Area… 
2011
2011
THE KEPLER LIGHT CURVES OF V1504 CYGNI AND V344 LYRAE: A STUDY OF THE OUTBURST PROPERTIES
We examine the Kepler light curves of V1504 Cyg and V344 Lyr, encompassing ∼736 days at one-minute cadence. During this span each… 
2011
2011
On the Progenitor System of Nova V2491 Cygni
Nova V2491 Cyg is one of just two detected pre-outburst in X-rays. The light curve of this nova exhibited a rare "re-brightening… 
2005
2005
submitted to the Astrophysical Journal Preprint typeset using L ATEX style emulateapj v. 11/12/01 A MODELING OF THE SUPER-EDDINGTON LUMINOSITY IN NOVA OUTBURSTS: V1974
  • 2005
  • Corpus ID: 11073046
2004
2004
Composite Accretion Disk and White Dwarf Photosphere Analyses of the FUSE and Hubble Space Telescope Observations of EY Cygni
We explore the origin of FUSE and Hubble Space Telescope STIS far-UV spectra of the dwarf nova EY Cygni during its quiescence… 
2000
2000
Period changes in W UMa-type eclipsing binaries: DK Cygni, V401 Cygni, AD Phoenicis and Y Sextantis
We present a period analysis of the four well- known W UMa-type eclipsing binaries DK Cyg (P = 0: 47), V401 Cyg (0: d 58), AD Phe… 
1976
1976
V1500 Cygni (nova Cygni 1975)
By clicking accept or continuing to use the site, you agree to the terms outlined in our Privacy Policy (opens in a new tab), Terms of Service (opens in a new tab), and Dataset License (opens in a new tab)