Main news about the GEOS
Pro-Am Conference on Stellar Astrophysics PDF Print E-mail
Written by Ennio Poretti   
Saturday, 31 March 2012 16:47
We will take the occasion offered by the

"Pro-Am Conference on Stellar Astrophysics",

planned from September 28th to October 1st, 2012 in Onet-Le-Chateau
(close to Rodez,  France), to have our annual GEOS meeting
on the same days.   We could discuss GEOS business on Friday
afternoon and/or Monday afternoon.  We strongly encourage
GEOS members

- to register to the Conference and
- to propose  talks

at the site

http://rr-lyr.ast.obs-mip.fr/capas2012/index.fr.php


The detailed agenda of the GEOS meeting will be fixed
among the registered participants. It will also be possible
to organize a technical workshop on the time-series analysis
after the Conference, very probably in Toulouse.
The  GEOS members interested in the technical workshop
are requested to contact  Jean-Francois Le Borgne and
Ennio Poretti in order to  evaluate the  feasibility.

Last Updated on Sunday, 01 April 2012 05:54
 
RRab Elements PDF Print E-mail
Written by Jean-François Le Borgne   
Wednesday, 06 October 2010 17:15

Following the exercise I made end of august by updating the elements of RR Lyr stars for the schedule of Tarot telescopes, I eventually updated the elements of 347 stars of the GEOS survey.

This is almost the whole sample of 356 stars. I just excluded a couple of stars for which detailed studies are on the way.

The result is in this file.

Most of the stars are RRab stars with the exception of 3 RRc and 2 misclassified cepheids in southern hemisphere. For some stars,new elements are not necessary: for these stars, the reference of the elements are given in the last column of the file. Again, these elements fit the recent observations made during the last decade.

They are intended to be used for predicting maxima in the near future. By the way, I made some statistics : During the last 7 years, after the start of RR Lyr program on the first Tarot telescope, the GEOS RR Lyr Survey collected 6062 CCD maxima on 356 stars.

Apart from the robotic telescopes, Tarot-Calern, Tarot-Chile and Alain Klotz' Faro, the observers who contributed are the following: N. Butterworth, L. Corp, E. Denoux, S. Dvorak, F. Fumagalli, F.-J. Hambsch, F. Hund, D. Husar, J.M. Llapasset, G. Maintz, J. Nicolas, M. Nobile, A. Paschke, P. de Ponthiere, P. Roblin, M. Serrau and F. Van Den Abbeel.

Jean-François Le Borgne

Last Updated on Wednesday, 06 October 2010 17:58
 
Other associations PDF Print E-mail
Written by Administrator   
Tuesday, 24 April 2007 18:55


  

Other Variable Star Associations


The American Association of Variable Star Observers (AAVSO)


The American Association of Variable Star Observers (AAVSO), founded in 1911, is the largest organization of variable star observers worldwide, with members in over 40 countries. Its purpose is to coordinate variable star observations made largely by dedicated amateur astronomers, evaluate the accuracy of these observations, compile, process, and publish them, and make them available to researchers, educators, and those who love variable stars. AAVSO Headquarters now receives over 350,000 observations yearly, from 550 observers worldwide, over half of whom live outside of the USA. They have compiled over 8.5 million observations of variable stars since the founding of the AAVSO in 1911.


Center for Backyard Astrophysics (CBA)


The Center for Backyard Astrophysics (CBA), has been founded in early 80's by Joseph Patterson. Since 1991 they have been engaged in long-term photometric studies of cataclismic variables (CV), mostly with CCD cameras mounted on small backyard telescopes. Amateurs from all around the world contribute to form a highly performing network of observatories, monitoring the activity of CV's over several days without interruption.


Association Française des Observateurs d'Étoiles Variables (AFOEV)

The French Association of Variable Star Observers (Association Française des Observateurs d'Étoiles Variables - AFOEV) was founded in 1921 on the initiative of Jean Mascart, then Director of Lyons Observatory, encouraged by Henri Grouiller, Marie Bloch (Lyons Observatory) and Antoine Brun, then Principal of an Elementary School at Le Breuil (Allier, France), with the collaboration of S.C. Hunter, the vice president of the American Association of Variable Star Observers (AAVSO). As from 1986, July 1, the association headquarters are at Strasbourg Observatory.
At the moment, the association numbers about a hundred observers from fifteen countries around the world.



British Astronomical Association Variable Star Section (BAAVSS)

The British Astronomical Association (BAA) was formed in 1890 and the Variable Star Section (VSS) the following year with the aim of collecting and analysing observations of variable stars. The section is run by a small group of officers who deal with various aspects separately but meet at intervals to discuss and decide future plans and policy. Feedback to members is through the VSS Circulars published four times a year and through the BAA Journal. Papers are published in the BAA Journal, the VSS Circulars and elsewhere. Gary Poyner is the director of the Variable Star Section of the British Astronomical Association.


 

Hungarian astronomical association

 

VSNET


 

BRNO-Variable Star Section of the Czech Astronomical Society


 

MEDUZA Variable stars group, in Czech Republic


 

The group of eclipsing binary observers of the Swiss Astronomical Society (BBSAG)

Last Updated on Friday, 26 June 2009 13:47
 
Wiki page updates - Nouvelles sur wiki page PDF Print E-mail
Written by Jean-François Le Borgne   
Wednesday, 22 September 2010 20:31

 

- VY CrB
After the observations made by Pierre de Ponthiere this year, we are able to show that VY CrB has a strong Blazhko effect (see attached figure: blue points, Pierre de Ponthiere; yellow points, Jean Marie Llapasset). Pierre's measurements combined with those made 3 years ago by Jean Marie and by Anton Paschke 10 years ago, allow to set the Blazhko period to 32 days. More details on the wiki page:
http://rr-lyr.ast.obs-mip.fr/dokuwiki/doku.php?id=vy_crb

Après les observations faites par Pierre de Ponthiere cette année, nous pouvons affirmer que VY CrB a un fort effet Blazhko (voir la figure attachée: points bleus: Pierre de Ponthiere; points jaunes: Jean Marie Llapasset). Les mesures de Pierre, combinées à celles de Jean Marie d'il y a 3 ans et celles d'Anton Paschke d'il y a 10 ans, permettent de fixer la période Blazhko à 32 jours. Plus de détails sur la page wiki:
http://rr-lyr.ast.obs-mip.fr/dokuwiki/doku.php?id=vy_crb

- RR Lyr:
The Blazhko effect of RR Lyr is fading as it was observed 50 years ago and as it probably does every 5-10 years ! The observations made by the VTT experiments (L. Corp, E. Denoux, A.+A. Klotz and myself) in 2008 and 2009 shows a variation of maximum O-Cs with an amplitude of about 0.09 day.  In 2010, this amplitude is 0.06 day only . We suspected this fading on the way last year but is confirmed this year. Also, the shapeof the O-Cs curve folded on Blazhko period becomes les and less sharp.
This is shown on the attached figure where the 2008 observations are in grey, the 2009 observations in purple. This year's maxima are shown in different colors corresponding to different Blazhko cycles. See VTT experiments page on the wiki:
http://rr-lyr.ast.obs-mip.fr/dokuwiki/doku.php?id=vtt_experiments .

L'effet Blazhko de RR Lyr décroit comme cela a été observé il y a 50 ans et comme cela se produit probablement tous les 5-10 ans ! Les observations faites avec les VTT (L. Corp, E. Denoux, A. Klotz et moi-même) en 2008 et 2009 montrent une variation des O-Cs des maximums avec une amplitude de l'ordre de 0.09 jour. En 2010, cette amplitude n'est plus que de 0.06 jour. Nous soupçonnions cette décroissance l'an dernier déjà, mais elle est confirmée cette année. Également, la forme de la courbe des O-Cs compositée sur la période Blazhko devient de moins en moins piquée. C'est ce que montre la figure attachée où les points de 2008 sont en gris, ceux de 2009 en pourpre. Les maxima de cette année sont en différentes couleurs correspondant aux différents cycles Blazhko. Voir la page des VTT sur le wiki:
http://rr-lyr.ast.obs-mip.fr/dokuwiki/doku.php?id=vtt_experiments

- Astropedia :I added a link in the wiki to the thesis of a colleague of mine, Thomas Gastine. His thesis might be of interest for most of us. It concerns the pulsation of cepheids
http://rr-lyr.ast.obs-mip.fr/dokuwiki/doku.php?id=stellarphysics_astro .
The text of the thesis may be downloaded from the Toulouse University library web site.

J'ai ajoute un lien dans le wiki sur la thèse d'un de mes collègues, Thomas Gastine. Sa thèse pourrait intéresser certains d'entre nous. Elle porte sur la pulsation des céphéïdes.
http://rr-lyr.ast.obs-mip.fr/dokuwiki/doku.php?id=stellarphysics_astro .
Le mémoire de la thèse peut être téléchargée depuis le site web de la bibliothèque de l'Université de Toulouse.

- Astropedia : I also included articles about heliocentric correction in the wiki.
http://rr-lyr.ast.obs-mip.fr/dokuwiki/doku.php?id=data_reduction .

Thesetextes are in English and French. They are also available on the pages http://rr-lyr.ast.obs-mip.fr/astropedia/

I also made a new design for the astronomical ephemeris http://rr-lyr.ast.obs-mip.fr/astro/astro.php

J'ai également introduit des articles sur la correction héliocentrique dans le wiki:
http://rr-lyr.ast.obs-mip.fr/dokuwiki/doku.php?id=data_reduction.

Ces textes sont en anglais et en français. Ils sont également disponibles depuis les pages http://rr-lyr.ast.obs-mip.fr/astropedia/.

Par ailleurs j'ai donné un nouveau look aux calculs astronomiques http://rr-lyr.ast.obs-mip.fr/astro/astro.php


I remember that the access to the wiki is open to anybody and to become a redactor one has to request for a login.


L'accès au wiki est ouvert mais pour devenir rédacteur, vous devez demander un login.

Jean-Francois Le Borgne

Last Updated on Wednesday, 06 October 2010 17:39
 
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