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Campaign to observe HR Lyrae

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Jeremy's picture
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Campaign to observe HR Lyrae

With Lyra becoming well placed for observation until the end of the year (at least in the northern hemisphere), we are launching a campaign to observe this old nova in quiescence. Coincidentally, this year is the centenary of the discovery of Nova Lyrae on 1919 December 6 by Miss Mackie at the Harvard College Observatory.

We are looking for nightly snapshot photometry (CCD or visual). In addition, some long time series photometry runs would be helpful. Spectroscopy is also desirable, but this will be a real challenge given the magnitude. I last observed it at V = 15.6 on April 1 at mag with the AAVSOnet’s SRO telescope.

Full details about the campaign, what is already known about HR Lyr and what we are seeking to discover about the star are available on the BAA website.

The campaign will continue until the end of the year

Jeremy Shears

Jeremy's picture
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Campaign update: 2019 May 10

We are now one month into the campaign and, whilst it’s still early days, it’s good to see the first data coming in. Many thanks to: David Boyd, Walter Cooney, Sjoerd Dufoer, Ian Miller, Ken Menzies, Martin Mobberley, Roger Pickard and Gary Poyner.

The star has varied between mag 15.4 and 16.2. Time series photometry by Roger Pickard and Ken Menzies has shown various humps and bumps in the light curve, but it’s too early to determine if they are periodic.

With Lyra becoming more accessible in the evening sky, I hope that further observations will begin to flow in. Do feel to join in the campaign. We are looking for nightly snapshot photometry to determine the overall shape of the light curve and well as some multi-hour photometry runs to look for short-term periodicities.

Further details about the campaign can be found here.

Robin Leadbeater's picture
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A spectrum

A very noisy low resolution ALPY 600 spectrum (It should be possible to do better) is similar to a low resolution 1981 spectrum from the literature.

 It shows a blue continuum with no obvious emission lines, though there is a hint of some small features common to both spectra

Cheers

Robin