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NC1119
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- Description:
-
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st1\:*{behavior:url(#ieooui) } /* Style Definitions */ table.MsoNormalTable {mso-style-name:'Tableau Normal'; mso-tstyle-rowband-size:0; mso-tstyle-colband-size:0; mso-style-noshow:yes; mso-style-parent:''; mso-padding-alt:0cm 5.4pt 0cm 5.4pt; mso-para-margin:0cm; mso-para-margin-bottom:.0001pt; mso-pagination:widow-orphan; font-size:10.0pt; font-family:'Times New Roman'; mso-ansi-language:#0400; mso-fareast-language:#0400; mso-bidi-language:#0400;} Normal 0 21 false false false MicrosoftInternetExplorer4 /* Style Definitions */ table.MsoNormalTable {mso-style-name:'Tableau Normal'; mso-tstyle-rowband-size:0; mso-tstyle-colband-size:0; mso-style-noshow:yes; mso-style-parent:''; mso-padding-alt:0cm 5.4pt 0cm 5.4pt; mso-para-margin:0cm; mso-para-margin-bottom:.0001pt; mso-pagination:widow-orphan; font-size:10.0pt; font-family:'Times New Roman'; mso-ansi-language:#0400; mso-fareast-language:#0400; mso-bidi-language:#0400;}In the present paper, the GEOS RR Lyr database ( Le Borgne et al., 2006 – 2007) is used to study the period variations of the best observed RR Lyrae stars belonging to the RRc sub-class.
- Submitted By:
- Joseph Remis (rms)
- Submitted On:
- 30 May 2022
- File Size:
- 145.29 Kb
- Downloads:
- 9
- File Author:
- Jacqueline Vandenbroere
- Submitted On:
- 23 May 2010
- Rating:
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