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AQL-208

Known as: AQL 208, AQL208 
National Institutes of Health

Papers overview

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2015
2015
There are few confirmed black holes with a mass of less ∼ 4 M ⊙ ?> and no neutron stars with masses greater than ∼ 2 M… 
2014
2014
We present data on 13 post-nova systems. This includes the recovery via UBVR photometry of the five post-novae X Cir, V2104 Oph… 
2012
2012
Recent spectropolarimetric studies of seven slowly pulsating B (SPB) and β Cep stars have suggested that photospheric magnetic… 
2012
2012
We present Spitzer Space Telescope mid-infrared IRS spectra, supplemented by ground-based optical observations, of the classical… 
2010
2010
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… 
2009
2009
We present new photometric data and analyze long-term UBV observations of three candidates for protoplanetary nebulae—F… 
2009
2009
We report the discovery of burst oscillations from the intermittent accretion-powered millisecond pulsar (AMP) HETE J1900.1-2455… 
Review
2004
Review
2004
We have surveyed 277 bright Be stars for short‐period (0.2–2 day) photometric variability using self‐correlation analysis of… 
Review
1981
Review
1981
It has been generally accepted that X-ray burst sources and other non-bursting ‘galactic bulge X-ray sources’ are low-mass close…