Hi Ross and all,

Yes I did exactly that.

This research is one of the reasons I was so happy to get Heystek on board
at HartRAO to improve our spectrometer. Better backends equal better (and
more) science.

Sorry I was trying to send this email to Andrew and did not check the cc
list.

Happy New Year all!

gordon

> I assume you removed the linear before performing the sine fit?
>
>
> On Fri, Dec 30, 2022, 6:09 PM Dr Gordon MacLeod <[email protected]>
> 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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