Wine and Cheese Fall 2022

This page records the schedule, titles and abstracts of the JHU/STScI CAS Astrophysics Wine & Cheese Series in Fall 2022.

Wine and Cheese sessions with one speaker will have a 50 minute talk with 10 minutes for questions. Sessions with two speakers will have two 25 minute talks, each with 5 minutes for questions. Sessions in the Graduate Student Series will have three 15 minute talks, each with 5 minutes for questions.

12 September

Ann Hornschemeier Cardif (GSFC/JHU)

The Proposed STAR-X MIDEX Mission
STAR-X is a MIDEX proposed to NASA in December 2021, that was recently (August 2022) selected for competitive Phase A study. Comprising an X-ray Telescope (XRT) provided by GSFC and MIT, a UV Telescope (UVT) provided by the University of Colorado, and a spacecraft provided by Ball Aerospace, STAR-X is designed to conduct time-domain sruvesy and to respond rapidly to transient events discovered by other observatories such as LIGO, Rubin/LSST, Roman/WFIRST, and SKA. STAR-X is a timely response to Astro2020’s recommendation for a space-based, sustaining time-domain and multi-messenger program. This talk will cover the mission and science case.

19 September

Carrie Filion (JHU)

Galactic Archaeology with the Subaru Prime Focus Spectrograph
The Subaru Prime Focus Spectrograph (PFS) will soon embark on an ambitious, multi-year survey that will investigate the nature of dark matter and study the formation and evolution of structure on a range of astrophysical scales. In this talk, I will provide a brief overview of the planned observations of individual, faint stars in the Local Group. I will detail the science motivating these observations and discuss the insight that we hope to gain.

Justin Otter (JHU)

Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past
Post-starburst galaxies (PSBs) have recently and rapidly quenched their star-formation, thus they are an important way to understand how galaxies transition from star-forming late-types to quiescent early-types. The recent discovery of large cold gas reservoirs in PSBs calls into question the theory that galaxies must lose their gas to become quiescent. Optical Integral Field Spectroscopy (IFS) surveys have revealed two classes of PSBs: central PSBs with central quenching regions and ring PSBs with quenching in their outskirts. We analyze a sample of 13 nearby ($z < 0.1$) PSBs with spatially resolved optical IFS data from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey and with matched resolution Atacama Large (sub-)Millimeter Array (ALMA) observations of $^{12}$CO(1-0). Disturbed stellar kinematics in 7/13 of our PSBs and centrally concentrated molecular gas is consistent with a recent merger for the majority of our sample. In galaxies without merger evidence, alternate processes may funnel gas inwards and suppress star-formation, including outflows, stellar bars, and minor mergers or interactions. The star-formation efficiencies of the post-starburst regions in nearly half our galaxies are suppressed while the gas fractions are consistent with star-forming galaxies. AGN feedback may drive this stabilization, and we observe AGN-consistent emission in the centers of 5/13 galaxies. Finally, our central and ring PSBs have similar properties except the ionized and molecular gas in central PSBs is more disturbed. Overall, the molecular gas in our PSBs tends to be compact and highly disturbed, resulting in concentrated gas reservoirs unable to form stars efficiently.

26 September

Thomas Essinger-Hileman (GSFC)

EXCLAIM: The EXperiment for Cryogenic Large-Aperture Intensity Mapping
The EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) will constrain star formation over cosmic time by carrying out a blind and complete census of redshifted carbon monoxide (CO) and ionized carbon ([CII]) emission in cross-correlation with galaxy survey data in redshift windows from the present to z=3.5 with a fully cryogenic, balloon-borne telescope. EXCLAIM will carry out extragalactic and Galactic surveys in a conventional balloon flight planned for 2023. EXCLAIM will be the first instrument to deploy µ-Spec silicon integrated spectrometers with a spectral resolving power R=512 covering 420-540 GHz. I will summarize the design, science goals, and status of EXCLAIM.

3 October

Namrata Roy (JHU)

Star Formation Suppression and Feedback in Nearby "Red Geyser" Galaxies
A key question in galaxy evolution is understanding how galaxies completely stop (or “quench”) their star formation towards the end of their lifetime. In spite of having the fuel necessary for forming stars, the lack of detected star formation in old massive galaxies indicates the presence of a feedback energy. Active galactic nuclei (AGN) driven feedback has been proposed to be the most efficient feedback mechanism capable of suppressing star formation - but direct evidence of such feedback in typical galaxies has been lacking. In this talk, I will present evidence from a series of papers that a new class of early-type galaxies, known as ‘red geysers’, may represent AGN feedback in action. I will show that these low redshift galaxies host low luminosity radio mode AGNs with signatures of large scale ionized gas outflows and suppressed star formation activities. These galaxies also frequently show signatures of inflowing cool neutral gas, possibly fueling the central AGN. I will present a multi-wavelength study of these red geyser population from a variety of observational datasets and discuss their role in the global quenching of star formation.

10 October

Yuan-Sen Ting (ANU)

Reconstructing Galaxy Merger History with Graph Neural Networks

17 October

Kalina Nedkova (STScI)

How Have Galaxies Grown Over the Last 10 Billion Years?
Signatures of the physical mechanisms that drive the formation pathways through which galaxies evolve are imprinted on their structure. In this talk, I will present how we have used a simultaneous multi-wavelength fitting approach to model the structure of HFF and CANDELS galaxies, which has allowed us to measure the sizes of faint, high redshift galaxies. Using these data, we have extended the stellar mass—size relation of galaxies over 0.2 ≤ z ≤ 2 to lower mass galaxies than previously studied at these redshifts. I will discuss key factors which may be responsible for driving the shape and evolution of the relations that we obtain. Finally, by modeling galaxies as a composition of bulges and disks, we can further investigate mass and size growth as a function of redshift not only of galaxies but individual galaxy components. I will conclude with some preliminary results showing the stellar mass—size relation of bulges and discs, and a brief discussion of the exciting prospects with JWST, Euclid, and the Nancy Grace Roman Telescope.

Samuel Grunblatt (JHU)

Planet Demographics from the Main Sequence to the Red Clump
Despite the recent discoveries of planets orbiting stars at all evolutionary stages, the evolution of planetary systems remains poorly understood. Studying planetary systems around subgiant and red giant stars is key to understanding how planetary systems change over time. The TESS 'Giants Transiting Giants' survey has yielded the detection of tens of planets and planet candidates orbiting subgiant and red giant stars. These planetary systems provide testbeds for understanding planet inflation and orbital decay, planet engulfment and potential chemical enhancement of host stars, and disruption of typical main sequence systems. Recent studies of the demographics of these systems have revealed that these systems display evidence for late-stage planet re-inflation (although the mechanism of this re-inflation is still up for debate), and a distribution of orbital eccentricities that may support evidence for planet-planet scattering and migration at late stages. Studying these systems as a function of stellar mass may resolve mysteries of giant planet formation as well. Extending the study of these systems to longer baselines will reveal the long-term stability of both hot Jupiters around rapidly evolving stars, as well as the longevity of Earthlike planets around Sunlike stars. Finally, studying these systems with the newest facilities can reveal new details of planetary system orbital and atmospheric evolution, as well as the occurrence of planets formed in other Galaxies.