Emission Line Variations in γ 2 Velorum
In this paper, we present results of an intensive search for periodic variations in the strength of the Hell emission line of �2 Vel relative to the nearby continuum. The data were obtained in 1986 and 1988 using an automated optical system located at the Amundsen-Scott South Pole Station. Ten of th...
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Cambridge University Press (CUP)
1991
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Online Access: | http://dx.doi.org/10.1017/s0074180900045113 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0074180900045113 |
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crcambridgeupr:10.1017/s0074180900045113 2024-03-03T08:36:38+00:00 Emission Line Variations in γ 2 Velorum Taylor, Mary Jane 1991 http://dx.doi.org/10.1017/s0074180900045113 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0074180900045113 en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms Symposium - International Astronomical Union volume 143, page 182-182 ISSN 0074-1809 journal-article 1991 crcambridgeupr https://doi.org/10.1017/s0074180900045113 2024-02-08T08:47:36Z In this paper, we present results of an intensive search for periodic variations in the strength of the Hell emission line of �2 Vel relative to the nearby continuum. The data were obtained in 1986 and 1988 using an automated optical system located at the Amundsen-Scott South Pole Station. Ten of the data sets have a time resolution between 2 and 3 minutes and consist of 2.3 - 20.4 hours of continuous photometry (Taylor, AJ, in press). Three of the data sets have a time resolution of about 1 minute and span between 1.2 and 6.5 hours. Article in Journal/Newspaper Amundsen-Scott South pole Cambridge University Press South Pole Amundsen-Scott ENVELOPE(0.000,0.000,-90.000,-90.000) Amundsen Scott South Pole Station ENVELOPE(0.000,0.000,-90.000,-90.000) Amundsen-Scott South Pole Station ENVELOPE(139.273,139.273,-89.998,-89.998) Symposium - International Astronomical Union 143 182 182 |
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Open Polar |
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Cambridge University Press |
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crcambridgeupr |
language |
English |
description |
In this paper, we present results of an intensive search for periodic variations in the strength of the Hell emission line of �2 Vel relative to the nearby continuum. The data were obtained in 1986 and 1988 using an automated optical system located at the Amundsen-Scott South Pole Station. Ten of the data sets have a time resolution between 2 and 3 minutes and consist of 2.3 - 20.4 hours of continuous photometry (Taylor, AJ, in press). Three of the data sets have a time resolution of about 1 minute and span between 1.2 and 6.5 hours. |
format |
Article in Journal/Newspaper |
author |
Taylor, Mary Jane |
spellingShingle |
Taylor, Mary Jane Emission Line Variations in γ 2 Velorum |
author_facet |
Taylor, Mary Jane |
author_sort |
Taylor, Mary Jane |
title |
Emission Line Variations in γ 2 Velorum |
title_short |
Emission Line Variations in γ 2 Velorum |
title_full |
Emission Line Variations in γ 2 Velorum |
title_fullStr |
Emission Line Variations in γ 2 Velorum |
title_full_unstemmed |
Emission Line Variations in γ 2 Velorum |
title_sort |
emission line variations in γ 2 velorum |
publisher |
Cambridge University Press (CUP) |
publishDate |
1991 |
url |
http://dx.doi.org/10.1017/s0074180900045113 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0074180900045113 |
long_lat |
ENVELOPE(0.000,0.000,-90.000,-90.000) ENVELOPE(0.000,0.000,-90.000,-90.000) ENVELOPE(139.273,139.273,-89.998,-89.998) |
geographic |
South Pole Amundsen-Scott Amundsen Scott South Pole Station Amundsen-Scott South Pole Station |
geographic_facet |
South Pole Amundsen-Scott Amundsen Scott South Pole Station Amundsen-Scott South Pole Station |
genre |
Amundsen-Scott South pole |
genre_facet |
Amundsen-Scott South pole |
op_source |
Symposium - International Astronomical Union volume 143, page 182-182 ISSN 0074-1809 |
op_rights |
https://www.cambridge.org/core/terms |
op_doi |
https://doi.org/10.1017/s0074180900045113 |
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Symposium - International Astronomical Union |
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143 |
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182 |
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182 |
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1792494518581329920 |