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Lasionycta arietis

Known as: Psammopolia arietis 
 
National Institutes of Health

Papers overview

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2017
2017
We thank Robert Wilson (University of Florida) for providing a custom version of his code to compute images of spotted stellar… Expand
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2013
2013
Two gram-negative, catalase- and oxidase-positive, bacillus-shaped bacterial strains were isolated from the semen of two rams… Expand
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2011
2011
We have used multi-epoch long-baseline radio interferometry to determine the proper motion and orbital elements of Algol and UX… Expand
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2007
2007
Aims. The RS CVn star UX Ari appears bluer when it is fainter, which is unusual for a spotted star; we aim to resolve this… Expand
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2005
2005
The Rieger periods are solar cycles with a time scale of months, which are present in both flaring activity and sunspot… Expand
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2005
2005
The high-resolution observation for RS CVn-type star UX Ari was carried out using echelle spectrograph of the 2.16m telescope at… Expand
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2001
2001
Here we present observational results on the RS CVn star UX Arietis from four very-long-baseline interferometry observations… Expand
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1993
1993
Observations of UX Arietis, in the range 9 mm - 21 cm, have been performed with the Effelsberg 100-m radio-telescope from… Expand
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1992
1992
Multifrequency observations of the quiescent radio emission of UX Arietis performed with the 100 m radio telescope of Effelsberg… Expand
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