Taophila sagittarii

 
National Institutes of Health

Topic mentions per year

Topic mentions per year

2000-2017
0120002017

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2017
2017
Context. Classical nova explosions occur on the surface of an accreting white dwarf in a binary system. After ejection of a… (More)
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2008
2008
We present broad-band 24, 70 and 160 μm photometry, 5-35 μm and 55-90 μm spectra of the eruptive variable V4332 Sgr from Spitzer… (More)
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2006
2006
We present the results of 11 nights of CCD unfiltered photometry of V4743 Sgr (Nova Sgr 2002 # 3) from 2003 and 2005. We find two… (More)
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2004
2004
We present optical observations of the enigmatic nova-like variable V4332 Sgr. The importance of this object should not be… (More)
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2004
2004
We use the PHOENIX code package to model the X–ray spectrum of Nova V4743 Sagittarii observed with the LETGS onboard the Chandra… (More)
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2003
2003
We present 1.2 mm continuum images and spectral line observations of CO(1–0) and SiO(3–2) rotational transitions of the recent… (More)
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2001
2001
Theoretical light curves of four recurrent novae in outburst are modeled to obtain various physical parameters. The four objects… (More)
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2000
2000
We report on the rapid X-ray variability of the variable star and X-ray transient V4641 Sagittarii (SAX J1819.3-2525 = XTE J1819… (More)
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