Mycoplasma aquilae

 
National Institutes of Health

Topic mentions per year

Topic mentions per year

2000-2014
012320002014

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2015
2015
Context. The parallax of pulsation, and its implementations such as the Baade-Wesselink method and the infrared surface… (More)
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2014
2014
We present the analysis of photometric and spectroscopic data of two classical Cepheids, FN Aquilae and V1344 Aquilae. Based on… (More)
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2008
2008
We have resolved the classical nova V1663 Aql using long-baseline near-IR interferometry covering the period from ∼5–18 days… (More)
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2006
2006
A total of 44 usable observations were made of three of the brightest Classical Cepheids in the sky, δ Cephei, η Aquilae and… (More)
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2003
2003
V1432 Aquilae (=RX J1940.2−1025) is the X-ray bright, eclipsing magnetic cataclysmic variable ∼37 ′ away from the Seyfert galaxy… (More)
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2003
2003
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The results of the CCD observations of the 2002 superoutburst of V1141 Aql are described. We have detected clear superhumps… (More)
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2002
2002
Direct diameter observations of Cepheid variables are used to calibrate the Barnes-Evans Cepheid surface brightness relation… (More)
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2000
2000
We have measured the diameters of the Cepheid variables δ Cephei (18 nights) and η Aquilae (11 nights) with the Navy Prototype… (More)
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2000
2000
The presence of the magnetic field on the classical Cepheidη Aquilae is established. The magnetic field shows periodic variations… (More)
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2000
2000
We present mean angular diameters for two cepheid variables, α Ursae Minoris and ζ Geminorum, determined with the Navy Prototype… (More)
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