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LPV Double Trouble Campaign

Stars we call Double Trouble are stars that have close companions that create difficulties for visual and CCD observers alike. 

Observers reporting the combined magnitude of both members of a pair are over estimating the brightness of the variable.

Observers reporting the magnitude of the close companion, when in fact, the variable has faded below the brightness of its insidious partner, create "flat bottom light curves", which do not represent the actual behavioral characteristics of these stars.

We propose here, a long-term campaign on LPVs that are Double Trouble.

The initial goals of the campaign are as follows:

1- To raise awareness of the trouble they cause, and the affect it has on AAVSO data. We hope that bringing attention to these stars will cause observers to submit more accurate data. A side project in this campaign is to have a note regarding these special situations appear in the footer of every AAVSO chart plotted for them to assist in bringing these devils into the light.

2- Determine true minima of the variable members of these close pairs. Not all of these characteristics are well-known, or correctly listed in various catalogs.

3- Increase the density of coverage in hopes of characterizing these stars throughout their light cycles, not just at minimum. 

4- We also hope to create a program that utilizes the strengths of both visual and CCD observers working together. Visual observers providing intense coverage in the bright range of the stars, with occasional data provided by CCD observers, and CCD observers picking up the coverage when these stars get below the typical threshold for visual observations (<13.5).

5- Provide an observing challenge that is as much fun for the challenge as it is for the potential scientific payoff. Observing and splitting close double stars has been enjoyed as part of the traditional hobby space of observational astronomy for hundreds of years. These close pairs have the added advantage of never looking the same way twice, since at least one of the members is variable!  

As we learn more about these stars we may expand the goals of the campaign to include any serendipitous discoveries made along the way, and we will certainly expand the list of stars as more are brought to our attention. If you know of any LPVs (or other types of stars) with close companions that may affect the accuracy of the data submitted to the AAVSO please contact the section leader, Mike Simonsen at mikesimonsen at aavso.org.

The campaign list (sorted by RA) for February 2012 follows:

SV And

00 04 20.07 +40 06 35.8 

7.7-14V

S Ori

05 29 00.90 -04 41 32.8

7.2-14V

Z Tau

05 52 24.86 +15 47 43.8

9.8-18.0V

ST Aur

06 14 59.05 +46 47 47.5

11.5-<15.0V

VV Gem

06 25 56.00 +25 32 24.3

12.0-<16.2p

S Lyn

06 44 34.11 +57 54 39.9

8.5-14.8V

SY CMa

07 10 33.08 -19 50 10.7

8.7-14.1:V

WX CMi

07 11 57.45 +07 29 59.3

11.0-19V

TT Mon

07 25 40.63 -05 51 01.3

7.2-14.4V

T CMi

07 34 00.47 +11 44 07.2

9.5-15.1V

RR Vir

14 04 53.43 -09 11 41.2

10.7-17.5V

X Dra

18 06 52.23 +66 09 19.2

8.9-15.8V

Z Lyr

18 59 36.80 +34 57 16.3

9.2-15.3V

WZ Lyr

19 02 15.03 +47 12 59.7

9.7-15.5V

UU Lyr

19 05 42.35 +28 05 00.0

11.5-<16.1p

ST Lyr

19 09 45.56 +43 36 53.3

10.6-<18V

TU Aql

19 27 36.35 +02 03 10.8

8.5-14.6V

YZ Vul

19 44 02.14 +27 46 05.8

9.0-16.8V

SW Aql

19 50 40.68 +12 49 11.9

11.9-<14.5V

ST Sge

20 11 42.18 +20 37 17.0

10.0-14.9V

FG Sge

20 11 56.06 +20 20 04.4

9.4-13.6B

RR Aqr

21 15 01.28 -02 53 45.2

9.1-14.7V

LX Cyg

21 55 57.07 +48 20 50.9

11.5-<17.0V

DG Peg

22 03 33.92 +14 00 31.2

10.4-14.5V

 

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Mike Simonsen,
Feb 3, 2012, 1:02 PM
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