AAVSO: NGC 6811 Observing Campaign

Designation	AAVSO Name	VSX Link (for more info)	Comments
1932+46	NSV 12196	Click
1938+46	NSV 12304	Click
1937+46B	NSV 12298	Click
1934+46A	6811 V01	Click	van Cauteren, et al. Comm. in Asteroseismology 146 (2005)
1934+46B	6811 V02	Click	van Cauteren, et al. Comm. in Asteroseismology 146 (2005)
1934+46C	6811 V03	Click	van Cauteren, et al. Comm. in Asteroseismology 146 (2005)
1934+46D	6811 V04	Click	van Cauteren, et al. Comm. in Asteroseismology 146 (2005)
1934+46E	6811 V05	Click	van Cauteren, et al. Comm. in Asteroseismology 146 (2005)
1935+46A	6811 V06	Click	van Cauteren, et al. Comm. in Asteroseismology 146 (2005)
1935+46B	6811 V07	Click	van Cauteren, et al. Comm. in Asteroseismology 146 (2005)
1933+46B	6811 V08	Click	van Cauteren, et al. Comm. in Asteroseismology 146 (2005)
1933+46C	6811 V09	Click	van Cauteren, et al. Comm. in Asteroseismology 146 (2005)
1931+45	RXJ1934+45	Click	Akerlof, et al. (2001) - ROTSE survey for variables
1933+46	CTM3 CYG	Click	Schweitzer, par Emile. Bull. AFOEV #98
The following stars are somewhat close to NGC 6811. We list them here as secondary targets should you want to observe them while near the NGC6811 field. But please do not observe them in lieu of your normal NGC 6811 observations.
1937+46	BR Cyg	Click	AAVSO Chart & Shawn Dvorak's (DKS) EB Ephemeris Generator or Kreiner
1931+47	V796 Cyg	VSX	Shawn Dvorak's (DKS) EB Ephemeris Generator or Kreiner
1930+46	V894 Cyg	V894 Cyg	Shawn Dvorak's (DKS) RR Lyr Ephemeris Generator

Recent Information

Image from CWST - Sep 2, 2006. The CCD is actually continuous and the two halfs are joined but the data are stored with overscan regions in the middle. So think of them as an image which is joined straight across, so ignore the middle because it is not a real gap. Image is unreduced with different bias levels. Click for the full image.

Light curves of some of the variables as of Sep. 1:
6811 V01
6811 V02
6811 V03
6811 V04
6811 V05
CTM3 CYG

search engine | site map | links | contact us