I assume you removed the linear before performing the sine fit?

On Fri, Dec 30, 2022, 6:09 PM Dr Gordon MacLeod <g...@hartrao.ac.za> wrote:

> Hi Andrew,
>
> Hope you are enjoying your Christmas break, Merry Christmas!
>
> I thought I'd share with you an image I've recently created on excited-OH
> masers at 6.035 GHz, see attached. This is not yet published nor released
> data.
>
> These are fitted gaussian profiles to a Zeeman pair. You can easily see
> the cyclical undulation.
>
> I fitted a sinusoid to this and found a period of 360.3+/-0.5 Days and NOT
> 365 days. It is not yet conclusive; more data is required.
>
> There are 3 potential possibilities to explain these results.
>
> 1. The period is 365 days and there is a source about 30-40 arcsec away
> from the beamcenter - it's possibly a baricentric/heliocentric vlsr
> correction issue.
>
> 2. It is two Zeeman pairs line-blended and one or both are periodic.
>
> and
>
> 3. It is a gravitational effect, the result of masers associated with a
> binary - when the YSOs are aligned the velocities closer...
>
> I cannot find an object at about 30" but maybe it's there. I think it is
> option 2 to be honest.
>
> Of coarse there can be other explanations but they become less and less
> likely.
>
> More to the point, this result demonstrates the sensitivity of monitoring
> masers and velocity drift. This is a new line of research worth continuing
> and using more observatories.
>
> Who knows what it will turn up.
>
> Regardless, thought of our conversation in SA when I first saw it.
>
> All the best in 2023, Happy New Year!
>
> gordon
>
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