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This episode is special in many ways. Not only do I have a mega-interesting and inspiring guest on this episode, we're also having our conversation in English for the first time in this podcast's short history. And if that wasn't enough, my microphone gave up, which led to my voice having a "canned" tone this time. I hope you can ignore that and instead be fully inspired by and take part in loads of interesting thoughts, reflections and topics.Johnny Oduya is a two-time Stanley Cup champion with the Chicago Blackhawks. Olympic silver medalist and World cup bronze with Team Sweden. Close to 1000 games at NHL level. When I'm asked who's the best player I have coached, I usually answer his name. Not only because of his achievements and titles, but mainly because of his personality. His dedication, determination and his intense passion to be challenged, to explore and to improve. I have probably never met a person who has worked as hard with such purpose as him. Today Johnny is a successful entrepreneur with his companies Hale and Atunya and many exciting projects underway.We talk about “From Västerbron to Café opera”. We talk about Identity, Awareness, Resilience, Chicago Blackhwaks and much more. Hosted on Acast. See acast.com/privacy for more information.

Great questions and observations tonight from Orange County California. From V in Sweden And after I listen to that show with Tom and Gaby I come a cross this article ourorganicwellness.com/amish-f… so they is trying to take our good foods away from us Donate to Fakeologist | Fakeologist Live show schedule | Audio archives | […]

 Vì sao tôi phải đầu hàng?Đầu hàng có nghĩa là thua cuộc? Cái Tôi Giả Tạo ( False Self) là gì? Trong tập này chúng ta sẽ cùng chia sẻ về những câu hỏi trên. Mong rằng sau tập này chúng ta sẽ có thêm những suy nghĩ và quyết định tích cực cho chính bản thân mình trong các mối quan hệ và tương tác xã hội. Hãy share nếu bạn thấy podcast này giúp ích cho bạn :) Love,From Vân & Trân #TamLyOi

We meet Professor Riikka Puurunen of Aalto University in Finland, and discuss the history of ALD and other topics close to her heart.  You may also wish to check out the articles we mentioned on this episode:  A Short History of Atomic Layer Deposition: Tuomo Suntola's Atomic Layer Epitaxy, Riikka Puurunen https://onlinelibrary.wiley.com/doi/full/10.1002/cvde.201402012   From V. B. Aleskovskii's “Framework” Hypothesis to the Method of Molecular Layering/Atomic Layer Deposition, Anatolii A. Malygin et al. https://doi.org/10.1002/cvde.201502013 

For more information please email me at orpagan@yahoo.com or leave a comment at baldscientist.com. I can also be reached on Twitter: @baldscientist. Credits, Acknowledgments, and References Introduction courtesy of Mr. Micah Hanks. Strange Survivors: How Organisms Attack and defend in the Game of Life. BenBella Books. Copyright 2018 Oné R. Pagán. The First Brain: The Neuroscience of Planarians. Oxford University Press. Copyright 2014 Oné R. Pagán. Mr. Peter Cawdron's website: thinkingscifi.wordpress.com. “Not explaining science…” From Carl Sagan's “The Demon-Haunted World: Science as a Candle in the Dark”. Ballantine Books, 1996. "Revolutionary new drugs..." From E. O. Wilson's "The future of life". Vintage, 2003. "The heart has his reasons..." From Pascal's "Pensees" "Any single brain, including yours..." From V. S. Ramachandran's "The tell-tale brain". Norton 2012. "It is essential to understand our brains..." From F. Crick's "The astonishing hypothesis". Scribner, 1995. "Planarians are rather wonderful and challenging beasts..." From J. McConnell's "Manual of psychological experimentation on planarians", Self-published, 1967 Music courtesy of YouTube Audio Library. Fanfare sounds courtesy of freesoundeffect.net. • changizi.com • phenomena.nationalgeographic.com/blog/laelaps/ • scienceblogs.com/laelaps/2010/03/15/so-you-want-to-write-a-pop-sci/ • phenomena.nationalgeographic.com/2010/03/16/so-you-want-to-write-a-pop-sci-book-part-2-the-value-of-blogs • www.wired.com/wiredscience/2010/03/so-you-want-to-write-a-pop-sci-book-part-3-writing-the-damn-thing • psychologytoday.com/blog/nature-brain-and-culture/201009/how-write-popular-science-book The opinions expressed by me or my guests do not necessarily represent the opinions and policies of my employer, West Chester University of Pennsylvania, my family, our dog, Ginger, or Charles Darwin. --- This episode is sponsored by · Anchor: The easiest way to make a podcast. https://anchor.fm/app --- Send in a voice message: https://anchor.fm/one-r-pagan/message

From V-2 to Saturn V... and all that came with it...NuzBox - Coffee with Curmudgeons - February 19 2018The views, opinions and conclusions expressed in this show are those of the creator, organization or guests and not necessarily those of NuzBox, it’s staff or its officers and trustees. The show has not been reviewed or approved by NuzBox and the creator, organization or guests is solely responsible for its content. Any resemblance to persons, living or dead, is entirely coincidental or is intended purely as a satire, parody or spoof of such persons and is not intended to communicate any true or factual information about that person.

This week on Promoter 101 Steiny chats with Works Entertainment's David Britz and Straight No Chaser's Seggie Isho and David Roberts after their final show of the tour in Maui. Plus we are joined by two of the venue world's who’s who The T-Mobile Arena’s Sid Greenfeig and The Denver Levitt Pavilion’s Chris Zacher. A bonus segment with Scott Perry filling us all in on the music tech world From V.R. to Amazon's Alexa. Dan and Luke break down the news of the week with Amplify Media's Dave Brooks.

This week on Promoter 101 Steiny chats with Works Entertainment's David Britz and Straight No Chaser's Seggie Isho and David Roberts after their final show of the tour in Maui. Plus we are joined by two of the venue world's who’s who The T-Mobile Arena’s Sid Greenfeig and The Denver Levitt Pavilion’s Chris Zacher. A bonus segment with Scott Perry filling us all in on the music tech world From V.R. to Amazon's Alexa. Dan and Luke break down the news of the week with Amplify Media's Dave Brooks.

In the current cosmological scenario clusters, that are the biggest virialized systems of the Universe, are formed through accretion of smaller objects from the cosmic web in which they are embedded. During these events the galaxies involved are modified due to interaction with other galaxies, the cluster hot X-ray emitting gas and the cluster potential well. Some of mechanisms acting in dense environments are tidal stripping, mergers and ram pressure stripping, just to name a few. These mechanisms involved in galaxy evolution are also responsible for the formation of what is called the intracluster light (ICL). ICL consists of stars in clusters that are not bound to any cluster member. Numerical simulations predict that the stars contributing to the ICL component are unbound by the processes that are involved in galaxy evolution and in the formation of the brightest cluster cD galaxies in particular. The aim of this work is to study the ICL component in the central core of Hydra I. Hydra I is a medium compact cluster in the Southern Hemisphere at a distance of 50 Mpc. The cluster, a relaxed system from X-ray observations, is dominated by two non interacting elliptical galaxies, NGC 3311 (cD) and NGC 3309 (E3). We are interested in the kinematic relation between the ICL component and the cD halo of NGC 3311 and in exploring what can be understood from the photometric and kinematic characteristics of the ICL about the evolutionary history of the cluster as a whole. We studied the core of Hydra I using three different kinds of data. With UT1-FORS2 longslit spectroscopy we investigated the absorption line kinematics of NGC 3311. With UT1-FORS2 multislit-imaging spectroscopy we probed the kinematics of the Planetary Nebulas (PNs) tracing the stellar light in the central 100 × 100 kpc2 of the cluster, around NGC 3311. Finally, with WFI-ESO2.2m telescope photometry we studied the light distribution around the cD galaxy and its substructures. The absorption line kinematics of NGC 3311 shows that the stellar halo of NGC 3311 is dominated by the central intracluster stars of the cluster. The transition from predominantly galaxybound stars to cluster stars occurs in the radial range from 4 to 12 kpc from the center of the galaxy. The diffuse light in the Hydra I cluster is still un-mixed. The PN line-of-sight velocity distribution (LOSVD) shows a multi-peaked structure and reveals the presence of subcomponents in the cluster core. From V-band photometric data we discovered an excess of light, with respect to a symmetric distribution, in the North-East part of the halo of NGC 3311. The excess has a velocity compatible with the velocity of the PNs contributing to a high-velocity peak in the PN LOSVD and a group of dwarf galaxies populating the central core of the Hydra I cluster. The excess of light could have formed from stars unbound from the small group of dwarf galaxies that were partially disrupted during a recent close passage through the dense cluster core and which are now behind NGC 3311. The stellar population and structural properties of one of the DWs, HCC 26, are consistent with those of other dwarf elliptical galaxies. We conclude that even if from X-rays Hydra I appears to be the prototype of a relaxed and dynamically evolved cluster, the build up of the diffuse light and halo of its central cD galaxy, NGC 3311, is still ongoing.