Search Publications

Star Formation Suppression by Tidal Removal of Cold Molecular Gas from an Intermediate-redshift Massive Post-starburst Galaxy
DOI: 10.3847/2041-8213/ac75ea Bibcode: 2022ApJ...936L..11S

Bezanson, Rachel; Kriek, Mariska; Greene, Jenny E. +7 more

Observations and simulations have demonstrated that star formation in galaxies must be actively suppressed to prevent the formation of overly massive galaxies. Galactic outflows driven by stellar feedback or supermassive black hole accretion are often invoked to regulate the amount of cold molecular gas available for future star formation but may …

2022 The Astrophysical Journal
eHST 18
The homogeneity of chemical abundances in H II regions of the Magellanic Clouds
DOI: 10.1093/mnras/stac2974 Bibcode: 2022MNRAS.517.4497D

García-Rojas, J.; Esteban, C.; Rodríguez, M. +2 more

We use very deep spectra obtained with the Ultraviolet-Visual Echelle Spectrograph at the Very Large Telescope to derive physical conditions and chemical abundances of four H II regions of the Large Magellanic Cloud (LMC) and four H II regions of the Small Magellanic Cloud (SMC). The observations cover the spectral range 3100-10400 Å with a spectr…

2022 Monthly Notices of the Royal Astronomical Society
eHST 18
A complex multiphase DLA associated with a compact group at z = 2.431 traces accretion, outflows, and tidal streams
DOI: 10.1093/mnras/stac1824 Bibcode: 2022MNRAS.514.6074N

Charlton, Jane C.; Kacprzak, Glenn G.; Churchill, Christopher W. +4 more

As part of our program to identify host galaxies of known z = 2-3 Mg II absorbers with the Keck Cosmic Web Imager (KCWI), we discovered a compact group giving rise to a z = 2.431 DLA with ultrastrong Mg II absorption in quasar field J234628+124859. The group consists of four star-forming galaxies within 8-28 kpc and v ~ 40-340 km s-1 of…

2022 Monthly Notices of the Royal Astronomical Society
eHST 18
Evidence of a complex structure within the 2013 August 19 coronal mass ejection. Radial and longitudinal evolution in the inner heliosphere
DOI: 10.1051/0004-6361/202142966 Bibcode: 2022A&A...662A..45R

Jian, L. K.; Rodríguez-Pacheco, J.; Zouganelis, I. +9 more

Context. Late on 2013 August 19, a coronal mass ejection (CME) erupted from an active region located near the far-side central meridian from Earth's perspective. The event and its accompanying shock were remotely observed by the STEREO-A, STEREO-B, and SOHO spacecraft. The interplanetary counterpart (ICME) was intercepted by MESSENGER near 0.3 au …

2022 Astronomy and Astrophysics
SOHO 18
Kinematic footprint of the Milky Way spiral arms in Gaia EDR3
DOI: 10.1093/mnras/stac642 Bibcode: 2022MNRAS.512.1574M

Pérez-Villegas, Angeles; Martinez-Medina, Luis; Peimbert, Antonio

The Milky Way spiral arms are well established from star counts as well as from the locus of molecular clouds and other young objects; however, they have only recently started to be observed from a kinematics point of view. Using the kinematics of thin disc stars in Gaia EDR3 around the extended solar neighbourhood, we create x-y projections colou…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 18
METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble Program. IV. Calibration of Dust Depletions versus Abundance Ratios in the Milky Way and Magellanic Clouds and Application to Damped Lyα Systems
DOI: 10.3847/1538-4357/ac7713 Bibcode: 2022ApJ...935..105R

Jenkins, Edward B.; Yanchulova Merica-Jones, Petia; Gordon, Karl D. +9 more

The evolution of the metal content of the universe can be tracked through rest-frame UV spectroscopy of damped Lyα systems (DLAs). Gas-phase abundances in DLAs must be corrected for dust depletion effects, which can be accomplished by calibrating the relation between abundance ratios such as [Zn/Fe] and depletions (the fraction of metals in gas, a…

2022 The Astrophysical Journal
eHST 18
Coronal Mass Ejection Deformation at 0.1 au Observed by WISPR
DOI: 10.3847/1538-4357/ac90bf Bibcode: 2022ApJ...938...13B

Vourlidas, Angelos; Stenborg, Guillermo; Hess, Phillip +3 more

Although coronal mass ejections (CMEs) resembling flux ropes generally expand self-similarly, deformations along their fronts have been reported in observations and simulations. We present evidence of one CME becoming deformed after a period of self-similar expansion in the corona. The event was observed by multiple white-light imagers on 2021 Jan…

2022 The Astrophysical Journal
SOHO 18
Near-Earth Sub-Alfvénic Solar Winds: Interplanetary Origins and Geomagnetic Impacts
DOI: 10.3847/1538-4357/ac4471 Bibcode: 2022ApJ...926..135H

Hajra, Rajkumar; Tsurutani, Bruce T.

The near-Earth solar wind is in general super-Alfvénic and supermagnetosonic. Using all available near-Earth solar wind measurements between 1973 and 2020, we identified 30 intervals with sub-Alfvénic solar winds. The majority (83%) of the events occurred within interplanetary coronal mass ejection magnetic clouds (MCs)/driver gases. These MC sub-…

2022 The Astrophysical Journal
SOHO 18
Deep learning-based super-resolution and de-noising for XMM-newton images
DOI: 10.1093/mnras/stac2437 Bibcode: 2022MNRAS.517.4054S

Valtchanov, Ivan; Verdugo, Eva; Lieu, Maggie +6 more

The field of artificial intelligence based image enhancement has been rapidly evolving over the last few years and is able to produce impressive results on non-astronomical images. In this work, we present the first application of Machine Learning based super-resolution (SR) and de-noising (DN) to enhance X-ray images from the European Space Agenc…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 18
Quasi-periodic Accelerations of Energetic Particles during a Solar Flare
DOI: 10.3847/2041-8213/ac6fd2 Bibcode: 2022ApJ...931L..28L

Chen, Wei; Li, Dong

We report the observation of nonstationary quasi-periodic pulsations (QPPs) in high-energy particles during the impulsive phase of an X4.8 flare on 2002 July 23 (SOL2002-07-23T00:35). The X4.8 flare was simultaneously measured by the Reuven Ramaty High Energy Solar Spectroscopic Imager, Nobeyama Radio Polarimeters, and Nobeyama Radioheliograph. Th…

2022 The Astrophysical Journal
SOHO 18