Research Events
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Northwestern University

Weekly Astrophysics Seminars 2015-2016

Seminars are held at 4:00 PM on Tuesdays in Room F160
on the first floor of the Technological Institute (2145 Sheridan Road) unless otherwise noted


Fall Quarter 2015

  Date      Speaker / Seminar Host
  Sept. 22

Zhaohuan Zhu
   Princeton University
   Observational Signatures of Young Planets in Disks

Transitional disks are protoplanetary disks with gaps and holes. Although young planets can lead to gaps and holes in disks, recent near-IR polarization imaging (e.g. SEEDS, VLT) and submm (e.g. SMA, ALMA) observations have posed several puzzles. Such as, dust and gas seems to decouple in these disks and the decoupling can occur non-axisymmetrically in disks. Spiral patterns are also discovered in these disks. To understand these new findings, I have carried out hydrodynamic and magnetohydrodynamic global simulations with young planets in disks. Moreover, both dust particle dynamics and non-ideal MHD effects have been considered for the first time. By comparing such realistic simulations with observations, I have constrained protoplanetary disk properties and revealed the early stage of planet formation. Finally, I will discuss the observational strategies to directly find young planets in protoplanetary disks and suggest that accreting circumplanetary disks could be the key to detect young planets directly. I will argue that current direct imaging observations may have already found some circumplanetary disk candidates and there are more to come.

Sourav Chatterjee

  Sept. 29

Ryan Cooke
   University of California, Santa Cruz
   Finding the first metals in near-pristine environments

The birth of the first stars arguably marks one of the most important physical and chemical transformations of the Universe. These stars kick-started reionization and synthesised the first metals. However, despite their impact, we still know very little about them. Even though no primordial star has yet been identified, we can start to understand their properties by studying the relative abundances of the elements that were made during their lives. In this talk, I will present the results from a suite of model calculations that follow the enrichment of the first stars. These minihalo models predict the chemical signature that is borne into the second generation of stars, and provide a new perspective on the formation of carbon-enhanced metal-poor stars. I will also present the latest results from my survey to find the most metal-poor damped Lyman-alpha galaxies (1/1000 of solar metallicity) at redshift z~3. I show that some of these systems may have been enriched solely by the first generation of stars.

Claude-André Faucher-Giguère

  Oct. 6

Amaury Triaud
   Centre for Planetary Sciences, University of Toronto
   Hikes Across the Desert

Low mass stars, brown dwarfs and hot Jupiters have similar radii. For a fairly narrow size range (~0.7 to 2 Jupiter radii) Nature has produced objects covering nearly three orders of magnitude in mass (between 0.2 and 200 Jupiter masses). This is of particular importance for transit surveys which are mostly sensitive to size. Those same surveys are also heavily biased towards proximity to the central, most luminous object. This is how ground-based transit surveys have primarily found hot Jupiters. Those fascinating planets can at times be hotter and bigger than the smallest Hydrogen burning stars.

My talk will explore the transition from planet to brown dwarf, to low mass star, and how one can compare them to one another. I will show similarities, but also distinctions between these different classes of objects.

I will present the results of observations from the WASP survey including an independent and mostly unbiased confirmation of the brown dwarf desert. We also looked at the spin-orbit angle distributions, as measured from the Rossiter-McLaughlin effect, between both ends of that desert. They are very different. In addition, our observations discovered systems containing both planets and brown dwarfs that can make us wonder about their formation process.

Brown dwarfs, hot Jupiters and low mass stars have similar fluxes. I will show how colour-magnitude diagrams can be constructed to compare these objects and how they can used for observations. Their compilation unveiled a new diversity for exoplanets: they show a wider variety of atmospheric properties than their brown dwarf cousins.

Finally, I will push into the realm of circumbinary architectures, and how they can expand the discussion on the distinction between planets, brown dwarfs and low mass stars, but also how they can be exploited to study stellar and planetary formation, to investigate cold planetary atmospheres and help the search for and eventual characterisation of habitable-zone rocky worlds.

Yoram Lithwick

  Oct. 13

Tony Piro
   Carnegie Observatories

Vicky Kalogera

  Oct. 20

Thayne Currie
   Subaru Telescope/NAOJ

Fred Rasio

  Oct. 27

Tim Brandt
   Institute for Advanced Study
   High-Contrast Exoplanet Surveys: from Images to Spectra

Advances in adaptive optics and infrared instrumentation have allowed us to see young exoplanets millions of times fainter than their host stars at separations corresponding to the outer Solar system. Large surveys, including one by the international SEEDS collaboration, have searched for massive planets around a total of about 1000 stars. As I will show, the results of these surveys suggest that we are approaching the contrasts and separations needed to see young planets formed by core-accretion. Now, simple cameras are being replaced by integral-field spectrographs, and adaptive optics systems are being dramatically upgraded. Instruments like the CHARIS integral-field spectrograph for the Subaru telescope will improve our sensitivity to faint exoplanets while simultaneously allowing us to characterize their atmospheres in much more detail. All of these upgrades, particularly the transition from images to spectra, bring new and unsolved challenges in data analysis. I will give an overview of these challenges and the techniques we are developing to overcome them. We are now planning a two-year CHARIS survey to begin in early 2017. It will obtain low-resolution spectra of young giant planets, and will search about 100-150 stars for faint companions at separations as small as 0.1--0.2 arcseconds.

Vicky Kalogera

  Nov. 3

Raffaella Margutti
   Harvard University
   Eruptions, Disruptions and Explosions: Massive Stars at the End of their Lives

Vicky Kalogera

  Nov. 17

Maryam Modjaz
   New York University
   Stellar Forensics with Explosions: Supernovae, Gamma-Ray Bursts, and their Environments

Vicky Kalogera

  Nov. 24

Joop Schaye
   Leiden Observatory

Claude-André Faucher-Giguère

  Dec. 1

Yuan Li
   University of Michigan


For more information, contact: ciera@northwestern.edu

Past Astrophysics Seminars