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Mycoplasma aquilae

National Institutes of Health

Papers overview

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2018
2018
Near Infrared (NIR) and optical photometry and spectroscopy are presented for the nova V1831 Aquilae, covering the early decline… Expand
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2013
2013
Abundant concretions at two localities in central Colombia where the San Gil Inferior and San Gil Superior formations are exposed… Expand
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2011
2011
V1408 Aql (= 4U 1957+115) is a low-mass X-ray binary with an orbital period of nearly 9.3 hr, whose compact star is a black hole… Expand
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2010
2010
V605 Aquilae is today widely assumed to have been the result of a final helium shell flash occurring on a single-post-asymptotic… Expand
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2009
2009
We report observations of the eclipsing classical nova V368 Aql (Nova Aql 1936 No. 2). These data reveal that the orbital period… Expand
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2007
2007
We have resolved the classical nova V1663 Aql using long-baseline near-IR interferometry covering the period from ~5 to 18 days… Expand
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2002
2002
Direct diameter observations of Cepheid variables are used to calibrate the Barnes-Evans Cepheid surface brightness relation… Expand
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2001
2001
We have measured the diameters of the Cepheid variables δ Cephei (18 nights) and η Aquilae (11 nights) with the Navy Prototype… Expand
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2001
2001
We present observations of the classical nova V1425 Aquilae (Nova Aquila 1995) with the Infrared Space Observatory's (ISO) Short… Expand
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1991
1991
From a new spectroscopic orbit of the early-type binary system V 599 Aql, based on Reticon observations, we find : m p sin 3 i… Expand