BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//TYPO3/NONSGML News system (news)//EN
BEGIN:VEVENT
UID:news-25822@phys.au.dk
DTSTAMP:20210928T101442Z
DTSTART:20140917T131500Z
DTEND:20140917T140000Z
END:VEVENT
END:VCALENDAR




<div class="news news-single">
	<div class="article" itemscope="itemscope" itemtype="http://schema.org/Article">
		
	
			<script type="text/javascript">
				const showAllContentLangToken = "Vis alt indhold ";
			</script>

			
			

			<article class="typo3-delphinus delphinus-gutters">

				<!-- News PID: 83035 - used for finding folder/page which contains the news / event -->
				<!-- News UID: 25822 - the ID of the current news / event-->

				<div class="news-event">
					<div class="news-event__header">
						<!-- Categories -->
						
							<span class="text--stamp">
<!-- categories -->
<span class="news-list-category">
	
		
	
		
	
		
	
</span>

</span>
						

						<!-- Title -->
						<h1 itemprop="headline">General Physics Colloquium - Thomas M. Tauris: &#039;Millisecond Pulsars: Multifaceted Astrophysical Laboratories&#039;</h1>
						
					</div>

					

					<div class="news-event__content">

						<!-- Events info box -->
						
								

								<div class="news-event__info theme--dark" id="event-info">
									<h2 class="screenreader-only">Oplysninger om arrangementet</h2>

									
											<!--- Same date -->
											<div class="news-event__info__item news-event__info__item--time">
												<h3 class="news-event__info__item__header text--label-header">Tidspunkt</h3>
												<div class="news-event__info__item__content">
													<span class="u-avoid-wrap">
														Onsdag 17. september 2014,
													</span>
													<span class="u-avoid-wrap">
														&nbsp;kl. 15:15 -  16:00
													</span>
													<p class="news-event__info__item__ical-link"><a href="/aktuelt/nyhed/artikel/general-physics-colloquium-thomas-m-tauris-millisecond-pulsars-multifaceted-astrophysical-labo?tx_news_pi1%5Bformat%5D=ical&amp;type=9819&amp;cHash=c4b0a2df6740e9b7d2bcaab59a5befd1">Tilføj til kalender</a></p>
												</div>
											</div>
										

									<!-- Location detailed -->
									
											<!-- Location Simple -->
											
												<div class="news-event__info__item">
													<h3 class="news-event__info__item__header text--label-header">Sted</h3>
													<div class="news-event__info__item__content">
														<p>Fys. Aud.</p>
													</div>
												</div>
											
										

									<!-- Organizer detailed -->
									
											<!-- Organizer Simple -->
											
										

									<!-- Price -->
									

									<!-- Event link -->
									

									<!-- Registration -->
									
								</div>
							

						
							<!-- Media -->
							
								



							
						

						
							<div class="news-event__content__text">
								<span class="text--byline" id="byline">
									

									<!-- Author -->
									
										<span itemprop="author" itemscope="itemscope" itemtype="http://schema.org/Person">
											
													Af
												

											
													<a href="mailto:karin.vittrup@phys.au.dk">
														<span itemprop="name">Karin Vittrup</span>
													</a>
												
										</span>
									
								</span>

								

									<!-- Body text -->
									<h2>General Physics Colloquium</h2>
<p>&nbsp;
</p>
<p><strong>'Millisecond Pulsars: Multifaceted Astrophysical Laboratories'</strong>
</p>
<p>Thomas M. Tauris&nbsp;&nbsp;&nbsp;&nbsp;
</p>
<p>Universität Bonn / MPIfR
</p>
<p>&nbsp;
</p>
<p>Neutron stars are unique creations that allow for fundamental studies <br>in many disciplines of physics. Those which interact with a companion <br>star in a close binary system provide excellent astrophysical <br>laboratories with which to probe and improve our understanding of <br>stellar physics, supernova explosions, accretion processes and <br>gravitational wave sources. Radio millisecond pulsars are of special <br>interest since they are old neutron stars which have been spun-up to <br>very high rotation frequencies via accretion of mass and angular <br>momentum from a companion star. I will discuss the formation of <br>millisecond pulsars and demonstrate that their properties, revealed from <br>high-precision measurements, are fossil records of their past <br>evolutionary history and therefore provide an excellent playground for <br>theoretical modelling.<br><br>Caption: An artist's impression of an accreting X-ray millisecond <br>pulsar and its magnetosphere. [© NASA/Dana Berry]
</p>
<p>&nbsp;<img height="225" src="fileadmin/_migrated/RTE/RTEmagicC_PulsarCU0620.jpg.jpg" data-htmlarea-file-uid="14947" data-htmlarea-file-table="sys_file" width="400" alt>
</p>
<p><em>Wine and cheese will be served at 4 PM</em></p>
								
							</div>
						
					</div>

					
						<!-- Content elements -->
						
					
				</div>
			</article>

			
				
				
			

			<!-- related things -->
			
		

	</div>
</div>
