Search Publications

The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XXIV. Differences in Internal Kinematics of Multiple Stellar Populations
DOI: 10.3847/1538-4357/acaec6 Bibcode: 2023ApJ...944...58L

Brown, Thomas M.; Milone, Antonino P.; Vesperini, Enrico +12 more

Our understanding of the kinematic properties of multiple stellar populations (mPOPs) in Galactic globular clusters (GCs) is still limited compared to what we know about their chemical and photometric characteristics. Such limitation arises from the lack of a comprehensive observational investigation of this topic. Here we present the first homoge…

2023 The Astrophysical Journal
eHST 17
A Type II Radio Burst Driven by a Blowout Jet on the Sun
DOI: 10.3847/1538-4357/ace31b Bibcode: 2023ApJ...953..171H

Tian, Hui; Madjarska, Maria S.; Deng, Yuanyong +5 more

Type II radio bursts are often associated with coronal shocks that are typically driven by coronal mass ejections (CMEs) from the Sun. Here we conduct a case study of a type II radio burst that is associated with a C4.5-class flare and a blowout jet, but without the presence of a CME. The blowout jet is observed near the solar disk center in the e…

2023 The Astrophysical Journal
SOHO 17
Carbon Stars as Standard Candles: An Empirical Test for the Reddening, Metallicity, and Age Sensitivity of the J-region Asymptotic Giant Branch (JAGB) Method
DOI: 10.3847/1538-4357/acee69 Bibcode: 2023ApJ...956...15L

Lee, Abigail J.

The J-region Asymptotic Giant Branch (JAGB) method is a standard candle based on the intrinsic luminosities of carbon stars in the near-infrared. We directly constrain the impact of metallicity, age, and reddening on the JAGB method. We assess how the mode, skew, and spread of the JAGB star LF change throughout diverse stellar environments in M31'…

2023 The Astrophysical Journal
eHST 16
Gamma Cas Stars as Be+White Dwarf Binary Systems
DOI: 10.3847/2041-8213/acaaa1 Bibcode: 2023ApJ...942L...6G

Gies, Douglas R.; Wang, Luqian; Klement, Robert

The origin of the bright and hard X-ray emission flux among the γ Cas subgroup of B-emission line (Be) stars may be caused by gas accretion onto an orbiting white dwarf (WD) companion. Such Be+WD binaries are the predicted outcome of a second stage of mass transfer from a helium star mass donor to a rapidly rotating mass gainer star. The stripped …

2023 The Astrophysical Journal
eHST 16
The Green Bank North Celestial Cap Survey. VII. 12 New Pulsar Timing Solutions
DOI: 10.3847/1538-4357/acb43f Bibcode: 2023ApJ...944..154S

Ransom, S. M.; Kaplan, D. L.; McLaughlin, M. A. +22 more

We present timing solutions for 12 pulsars discovered in the Green Bank North Celestial Cap 350 MHz pulsar survey, including six millisecond pulsars (MSPs), a double neutron star (DNS) system, and a pulsar orbiting a massive white dwarf companion. Timing solutions presented here include 350 and 820 MHz Green Bank Telescope data from initial confir…

2023 The Astrophysical Journal
Gaia 16
CECILIA: The Faint Emission Line Spectrum of z 2-3 Star-forming Galaxies
DOI: 10.3847/2041-8213/ad07dc Bibcode: 2023ApJ...958L..11S

Maseda, Michael V.; Steidel, Charles C.; Law, David R. +7 more

We present the first results from Chemical Evolution Constrained Using Ionized Lines in Interstellar Aurorae (CECILIA), a Cycle 1 JWST NIRSpec/MSA program that uses ultra-deep ~30 hr G235M/F170LP observations to target multiple electron temperature-sensitive auroral lines in the spectra of 33 galaxies at z ~ 1-3. Using a subset of 23 galaxies, we …

2023 The Astrophysical Journal
JWST 16
X-Ray Detection of the Galaxy's Missing Baryons in the Circumgalactic Medium of L* Galaxies
DOI: 10.3847/2041-8213/acec70 Bibcode: 2023ApJ...955L..21N

Bianchi, S.; Piconcelli, E.; Nicastro, Fabrizio +10 more

The number of baryons hosted in the disks of galaxies is lower than expected based on the mass of their dark matter halos and the fraction of baryon-to-total matter in the Universe, giving rise to the so-called galaxy missing-baryon problem. The presence of cool circumgalactic matter gravitationally bound to its galaxy's halo up to distances of at…

2023 The Astrophysical Journal
XMM-Newton eHST 16
A Measurement of the Cosmic Optical Background and Diffuse Galactic Light Scaling from the R < 50 au New Horizons-LORRI Data
DOI: 10.3847/1538-4357/acaa37 Bibcode: 2023ApJ...945...45S

Cooray, Asantha; Zemcov, Michael; Symons, Teresa +2 more

Direct photometric measurements of the cosmic optical background (COB) provide an important point of comparison to both other measurement methodologies and models of cosmic structure formation, and permit a cosmic consistency test with the potential to reveal additional diffuse sources of emission. The COB has been challenging to measure from Eart…

2023 The Astrophysical Journal
Gaia eHST 16
Magnetic Activity Evolution of Solar-like Stars. I. S ph-Age Relation Derived from Kepler Observations
DOI: 10.3847/1538-4357/acd118 Bibcode: 2023ApJ...952..131M

van Saders, Jennifer; García, Rafael A.; Breton, Sylvain N. +9 more

The ages of solar-like stars have been at the center of many studies such as exoplanet characterization or Galactic-archeology. While ages are usually computed from stellar evolution models, relations linking ages to other stellar properties, such as rotation and magnetic activity, have been investigated. With the large catalog of 55,232 rotation …

2023 The Astrophysical Journal
Gaia 16
A New Study on a Type Iax Stellar Remnant and its Probable Association with SN 1181
DOI: 10.3847/1538-4357/acb138 Bibcode: 2023ApJ...944..120L

Hillier, D. John; Parker, Quentin A.; Ritter, Andreas +4 more

We report observations and modeling of the stellar remnant and presumed double-degenerate merger of Type Iax supernova Pa 30, which is the probable remnant of SN 1181 AD. It is the only known bound stellar SN remnant and the only star with Wolf-Rayet features that is neither a planetary nebula central star nor a massive Population I progenitor. We…

2023 The Astrophysical Journal
AKARI Gaia INTEGRAL XMM-Newton eHST 16