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Prikvačeni tweet
Have a mentioned I have a book (nearly) out?https://twitter.com/OUPAcademic/status/1156882302477012992 …
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Enjoying hearing about
@minervasouth from@austronomer today, but I wish I didn't get the same earworm everytime anyone mentions the town of Toowoomba.Hvala. Twitter će to iskoristiti za poboljšanje vaše vremenske crte. PoništiPoništi -
Oxford people: please help support the campaign to drop the graduate application fee. Motion for congregation on the 10th March - please turn up and vote!https://twitter.com/Ben_Sheldon_EGI/status/1224979070083129344 …
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Lots of work shows that these black holes are growing fast - Becky measures about 1 Solar mass per year inflow onto the BH. Theory says plenty of mechanisms - like gas moving along bars - can supply this amount of fuel.
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How do the supermassive black holes grow? What about by merging with other galaxies? Along with
@vrooje, Becky has studied a sample of bulgeless galaxies that haven’t had mergers - most of the BH growth isn’t from mergers, as it turns out.Prikaži ovu nitHvala. Twitter će to iskoristiti za poboljšanje vaše vremenske crte. PoništiPoništi -
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After a lot of work, she showed that galaxies that have AGN - growing black holes - are quenching rapidly and more recently. But does this mean AGN are causing quenching? Or just that quenching galaxies tend to host AGN?
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Becky’s PhD (blimey, she graduated three years ago!) was built around building a statistical model that tries to say how fast a galaxy is quenching (& for how long it’s been doing so) based on its colours.
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There are many possible causes of this band many of them are interrelated. This is a mess.pic.twitter.com/LEYZOmHBIu
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Her talk is focusing on why galaxies ‘quench’ - why they stop forming stars and turn from dynamic blue galaxies to red systems dominated by old stars.
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Excited to have
@drbecky_ giving her home Astro colloquium in @OxfordPhysics - a good chance for me to tweet what we’ve been working on.pic.twitter.com/sMVCvjmflK
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'Best until 2035' distracts from what should be a simple message: This is a great time to see Mars! Come see Mars! Everyone should see Mars! I want to spend interviews I do talking about that, not explaining exactly what the difference between one orbit and another is (6/6)
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By giving the 'not until 2035' line prominence, we set people up for disappointment. Because the truth is to anyone who isn't an expert, the view in 2022 will look basically the same (5/n)
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It's probably true that the 2020 close approach is closer than any other closest approach until the 30s - but the difference is so small it won't make any difference! (4/n)
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So far so good. But the press release and website make a big point of the fact that Mars won't be closer until 2033 (press release) or 2035 (website) (4/n)
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Mars during the week is about 80 million miles away - it's a few weeks after closest approach. (At closest approach, Mars will look better but it's lower earlier in the evening, which is prime time for family and public events) (3/n)
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The reason for choosing November is that it's a great time to see a nice, bright, close apparition of Mars in the evening sky. This is great - seeing Mars through a telescope is cool, and it really makes a difference when Mars is close. (2/n)
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Good news - the UK and
@RoyalAstroSoc are going to celebrate National Astronomy Week in November: https://astronomyweek.org.uk/ cc@natastroweek. For a grumpy astronomer take, read on (1/n)Prikaži ovu nitHvala. Twitter će to iskoristiti za poboljšanje vaše vremenske crte. PoništiPoništi -
Having
@ProjectPHaEDRA on@the_zooniverse is a joy - help the team understand the (often hidden) contribution made by early women astronomers. A few minutes of time will help!https://twitter.com/concreted0g/status/1222925258379923458 …
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I agree with Dallas. Enter Famelab, budding science communicators!https://twitter.com/FameLab/status/1222489819147853827 …
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