Search Publications

Molecular Gas Reservoirs in Massive Quiescent Galaxies at z 0.7 Linked to Late-time Star Formation
DOI: 10.3847/1538-4357/ac9af7 Bibcode: 2022ApJ...940...39W

Johnson, Benjamin D.; Bezanson, Rachel; Rieke, Marcia +6 more

We explore how the presence of detectable molecular gas depends on the inferred star formation histories (SFHs) in eight massive, quiescent galaxies at z ~ 0.7. Half of the sample have clear detections of molecular gas, traced by CO(2-1). We find that the molecular gas content is unrelated to the rate of star formation decline prior to the most re…

2022 The Astrophysical Journal
eHST 18
First Census of Gas-phase Metallicity Gradients of Star-forming Galaxies in Overdense Environments at Cosmic Noon
DOI: 10.3847/2041-8213/ac626f Bibcode: 2022ApJ...929L...8L

Teplitz, Harry I.; Fan, Xiaohui; Cai, Zheng +8 more

We report the first spatially resolved measurements of gas-phase metallicity radial gradients in star-forming galaxies in overdense environments at z ≳ 2. The spectroscopic data are acquired by the MAMMOTH-Grism survey, a Hubble Space Telescope (HST) cycle 28 medium program. This program is obtaining 45 orbits of WFC3/IR grism spectroscopy in the …

2022 The Astrophysical Journal
eHST 18
Detection of Intracluster Globular Clusters in the First JWST Images of the Gravitational Lens Cluster SMACS J0723.3-7327 at z = 0.39
DOI: 10.3847/2041-8213/ac990b Bibcode: 2022ApJ...940L..19L

Lee, Myung Gyoon; Jang, In Sung; Bae, Jang Ho

We present a survey of globular clusters (GCs) in the massive gravitational lens cluster SMACS J0723.3-7327 at z = 0.39 based on the early released JWST/NIRCam images. In the color-magnitude diagrams of the point sources, we clearly find a rich population of intracluster GCs that are spread over a wide area of the cluster. Their ages, considering …

2022 The Astrophysical Journal
JWST 18
Updated Photometry of the Yellow Supergiant Progenitor and Late-time Observations of the Type IIb Supernova SN 2016gkg
DOI: 10.3847/1538-4357/ac8a4c Bibcode: 2022ApJ...936..111K

Kilpatrick, Charles D.; Coulter, David A.; Foley, Ryan J. +4 more

We present Hubble Space Telescope (HST) observations of the Type IIb supernova (SN) SN 2016gkg at 652, 1698, and 1795 days from explosion with the Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3). Comparing to pre-explosion imaging from 2001 obtained with the Wide Field Planetary Camera 2, we demonstrate that SN 2016gkg is now fain…

2022 The Astrophysical Journal
eHST 18
Solar Energetic Particles Produced during Two Fast Coronal Mass Ejections
DOI: 10.3847/2041-8213/ac5b72 Bibcode: 2022ApJ...928L...6L

Wang, Yuming; Guo, Jingnan; Li, Xiaolei +1 more

Two recent extremely fast coronal mass ejections (CMEs) are of particular interest. The first one originated from the southern hemisphere on 2021 October 28 and caused strong solar energetic particle (SEP) events over a wide longitude range from Earth, STEREO-A, to Mars. However, the other one, originating from the center of the Earth-viewed solar…

2022 The Astrophysical Journal
SOHO 18
An Intensity Mapping Constraint on the CO-galaxy Cross-power Spectrum at Redshift 3
DOI: 10.3847/1538-4357/ac4888 Bibcode: 2022ApJ...927..161K

Marrone, Daniel P.; Keating, Garrett K.; Keenan, Ryan P.

The abundance of cold molecular gas plays a crucial role in models of galaxy evolution. While deep spectroscopic surveys of CO emission lines have been a primary tool for measuring this abundance, the difficulty of these observations has motivated alternative approaches to studying molecular gas content. One technique, line intensity mapping, seek…

2022 The Astrophysical Journal
eHST 18
Lyman Continuum Galaxy Candidates in COSMOS
DOI: 10.3847/1538-4357/ac3004 Bibcode: 2022ApJ...924...14P

Hathi, Nimish; Rafelski, Marc; Wang, Xin +11 more

Star-forming galaxies are the sources likely to have reionized the universe. As we cannot observe them directly due to the opacity of the intergalactic medium at z ≳ 5, we study z ~ 3-5 galaxies as proxies to place observational constraints on cosmic reionization. Using new deep Hubble Space Telescope rest-frame UV F336W and F435W imaging (30 orbi…

2022 The Astrophysical Journal
eHST 17
A Strong Shock During a Nova Outburst: An Origin of Multiple Velocity Systems in Optical Spectra and of High-energy Emissions
DOI: 10.3847/1538-4357/ac9475 Bibcode: 2022ApJ...939....1H

Kato, Mariko; Hachisu, Izumi

We propose a theoretical explanation of absorption/emission line systems in classical novae based on a fully self-consistent nova explosion model. We found that a reverse shock is formed far outside the photosphere (≳1013 cm) because later-ejected mass with a faster velocity collides with earlier-ejected matter. Optically thick winds bl…

2022 The Astrophysical Journal
Gaia 17
Discovery, Timing, and Multiwavelength Observations of the Black Widow Millisecond Pulsar PSR J1555-2908
DOI: 10.3847/1538-4357/ac49ef Bibcode: 2022ApJ...927..216R

Ransom, Scott M.; Michelson, P. F.; Halpern, Jules P. +21 more

We report the discovery of PSR J1555-2908, a 1.79 ms radio and gamma-ray pulsar in a 5.6 hr binary system with a minimum companion mass of 0.052 M . This fast and energetic ( $\dot{E}=3\times {10}^{35}$ erg s-1) millisecond pulsar was first detected as a gamma-ray point source in Fermi Large Area Telescope (LAT) sky survey o…

2022 The Astrophysical Journal
Gaia 17
Age Spreads and Systematics in λ Orionis with Gaia DR2 and the SPOTS Tracks
DOI: 10.3847/1538-4357/ac307f Bibcode: 2022ApJ...924...84C

Pinsonneault, Marc H.; Hillenbrand, Lynne A.; Cao, Lyra +1 more

In this paper we investigate the robustness of age measurements, age spreads, and stellar models in young pre-main-sequence stars. For this effort, we study a young cluster, λ Orionis, within the Orion star-forming complex. We use Gaia data to derive a sample of 357 targets with spectroscopic temperatures from spectral types or from the automated …

2022 The Astrophysical Journal
Gaia 17