We are excited to announce the launch of our new forums! You can access it forums.aavso.org. For questions, please see our blog post. The forums at aavso.org/forum have become read-only.
Announcement: New Applications
We are excited to announce the launch of our new applications! We're opening up early access to our new applications for searching, downloading, and submitting photometric observations. You can now access these applications through these links:
We ask for your feedback in order to help us improve these applications. Please send feedback for the applications above to feedback@aavso.org. Note: please avoid duplicating submissions across the two submit applications.
BH Cru, now clasified as spectral type SC, according to 'The evolutionary state of Miras with changing periods' by Uttenthaler et al is now properly a carbon star, spectral type C. The paper is an interesting read...
I found it interesting reading with discussions on Mira change types, spectroscopy, Tc, Li, convection and thermal pulses. The article even quoted AAVSO data and an AJ article from 2005 by Templeton, Mattei and Willson. Kevin Paxson - PKV
The article in question is: http://arxiv.org/pdf/1105.2198.pdf
I found it interesting reading with discussions on Mira change types, spectroscopy, Tc, Li, convection and thermal pulses. The article even quoted AAVSO data and an AJ article from 2005 by Templeton, Mattei and Willson. Kevin Paxson - PKV
I am especially fond of this star because of one of it's other names! :)
But it wasn't my discovery - it was Ronald G. Welch's discovery!
Cheers,
Doug