THE AMERICAN ASSOCIATION OF VARIABLE STAR OBSERVERS

Science ◽  
1916 ◽  
Vol 44 (1147) ◽  
pp. 898-898
Author(s):  
F. E. B.
Science ◽  
1917 ◽  
Vol 46 (1199) ◽  
pp. 620-621
Author(s):  
L. C.

1995 ◽  
Vol 155 ◽  
pp. 421-422 ◽  
Author(s):  
Janet A. Mattei

AbstractThe American Association of Variable Stars Observers is the world’s largest organization of variable star observers. Its services to the astronomical community and database on pulsating variables are described.


Science ◽  
1942 ◽  
Vol 96 (2496) ◽  
pp. 405-406
Author(s):  
L. CAMPBELL

2020 ◽  
Author(s):  
Stella Kafka

<p>The American Association of Variable Star Observers was formed in 1911 as a group of US-based amateur observers obtaining data in support of professional astronomy projects. Now, it has evolved into an International Association with members and observers from both the professional and non-professional astronomical community, actively supporting ground and space-based variable star projects. As such, the AAVSO’s main claim to fame is that it successfully engages backyard Astronomers, educators, students and professional astronomers in astronomical research, building inclusive international communities around its portfolio. I will present the main aspects of the association and how it has evolved with time to become a premium resource for variable star researchers. I will also discuss the various means that the AAVSO is using to support cutting-edge research, and give updates on the tools and resources that are now available to researchers worldwide.</p>


1993 ◽  
Vol 139 ◽  
pp. 425-427
Author(s):  
John R. Percy

AbstractSeveral types of cool pulsating variables show unexplained long-term changes in brightness, typically on time scales of 10 to 20 times the basic (pulsational) period. The visual and photoelectric programs of the American Association of Variable Star Observers (AAVSO) are well-suited for detecting and studying these changes. Some examples are given here, including yellow hypergiants, RV Tauri stars, small- and large-amplitude red giant and super giant variables. The study of pulsating variables on long time scales provides “new perspectives” on their behavior.


Science ◽  
1919 ◽  
Vol 49 (1262) ◽  
pp. 243-244
Author(s):  
L. C.

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