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AQL-208

Known as: AQL 208, AQL208 
National Institutes of Health

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Tretoquinol

Papers overview

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2015
2015
THE CASE FOR A LOW MASS BLACK HOLE IN THE LOW MASS X-RAY BINARY V1408 AQUILAE (= 4U 1957+115)
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
Life after eruption – IV. Spectroscopy of 13 old novae
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
CRITICAL EVALUATION OF MAGNETIC FIELD DETECTIONS REPORTED FOR PULSATING B-TYPE STARS IN LIGHT OF ESPaDOnS, NARVAL, AND REANALYZED FORS1/2 OBSERVATIONS
Recent spectropolarimetric studies of seven slowly pulsating B (SPB) and β Cep stars have suggested that photospheric magnetic… 
2012
2012
ELEMENTAL ABUNDANCES IN THE EJECTA OF OLD CLASSICAL NOVAE FROM LATE-EPOCH SPITZER SPECTRA
We present Spitzer Space Telescope mid-infrared IRS spectra, supplemented by ground-based optical observations, of the classical… 
2010
2010
THE OPTICAL ORBITAL LIGHT CURVE OF THE LOW-MASS X-RAY BINARY V1408 AQUILAE (= 4U 1957+115)
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
Pulsations and long-term photometric variability of three candidates for protoplanetary nebulae
We present new photometric data and analyze long-term UBV observations of three candidates for protoplanetary nebulae—F… 
2009
2009
DISCOVERY OF BURST OSCILLATIONS IN THE INTERMITTENT ACCRETION-POWERED MILLISECOND PULSAR HETE J1900.1-2455
We report the discovery of burst oscillations from the intermittent accretion-powered millisecond pulsar (AMP) HETE J1900.1-2455… 
Review
2004
Review
2004
Short‐Period Variable Be Stars Discovered or Confirmed through Self‐Correlation Analysis of Hipparcos Epoch Photometry
We have surveyed 277 bright Be stars for short‐period (0.2–2 day) photometric variability using self‐correlation analysis of… 
1987
1987
Soft X-ray transients in quiescence: observations of Aql X-1 and Cen X-4
Review
1981
Review
1981
A four-hour orbital period of the X-ray burster 4U/MXB1636—53
It has been generally accepted that X-ray burst sources and other non-bursting ‘galactic bulge X-ray sources’ are low-mass close… 
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