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Bothriocephalus scorpii

 
National Institutes of Health

Papers overview

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2018
2018
V923 Sco is a bright ($V$ = 5.91), nearby ($\pi$ = 15.46$\pm$0.40 mas) southern eclipsing binary. Because both components are… Expand
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2015
2015
We present optical and infrared spectroscopy of V1309 Sco, an object that erupted in 2008 in a stellar-merger event. During the… Expand
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2013
2013
The old nova V728 Sco has been recently recovered via photometric and spectroscopic observations, 150 yr after the nova eruption… Expand
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2012
2012
The highly eccentric Be binary system {delta} Sco reached periastron during early 2011 July, when the distance between the… Expand
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2012
2012
V921 Scorpii is a close binary system (separation 0025) showing the B[e]-phenomenon. The system is surrounded by an enigmatic… Expand
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2012
2012
Belonging to the group of B[e] stars, V921 Scorpii is associated with a strong infrared excess and permitted and forbidden line… Expand
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2011
2011
Context. Stellar mergers are expected to take place in numerous circumstences in the evolution of stellar systems. In particular… Expand
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2010
2010
Aims. Nova Scorpii 2008 was the target of our Director Discretionary Time proposal at VLT+UVES in order to study the evolution… Expand
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2007
2007
We report optical photometry and optical through mid-infrared spectroscopy of the classical nova V1186 Sco. This slowly… Expand
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2000
2000
Observations of the B0.2 V star q Scorpii have revealed unusual stellar wind characteristics: redshifted absorption in the far… Expand
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