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ALMA Observations of the Asymmetric Dust Disk around DM Tau
DOI: 10.3847/1538-4357/abe59f Bibcode: 2021ApJ...911....5H

Dong, Ruobing; Liu, Hauyu Baobab; Tsukagoshi, Takashi +5 more

We report an analysis of the dust disk around DM Tau, newly observed with the Atacama Large Millimeter/submillimeter Array (ALMA) at 1.3 mm. The ALMA observations with high sensitivity (8.4 µJy beam-1) and high angular resolution (35 mas, 5.1 au) detect two asymmetries on the ring at r ∼ 20 au. They could be two vortices in early …

2021 The Astrophysical Journal
Gaia 30
The ALMA Survey of 70 µm Dark High-mass Clumps in Early Stages (ASHES). IV. Star Formation Signatures in G023.477
DOI: 10.3847/1538-4357/ac2365 Bibcode: 2021ApJ...923..147M

Jackson, James M.; Sanhueza, Patricio; Lu, Xing +15 more

With a mass of ~1000 M and a surface density of ~0.5 g cm-2, G023.477+0.114, also known as IRDC 18310-4, is an infrared dark cloud (IRDC) that has the potential to form high-mass stars and has been recognized as a promising prestellar clump candidate. To characterize the early stages of high-mass star formation, we have obs…

2021 The Astrophysical Journal
Herschel 30
The Red Supergiant Binary Fraction as a Function of Metallicity in M31 and M33
DOI: 10.3847/1538-4357/abd47b Bibcode: 2021ApJ...908...87N

Neugent, Kathryn F.

Recent work measuring the binary fraction of evolved red supergiants (RSGs) in the Magellanic Clouds points to a value between 15% and 30%, with the majority of the companions being unevolved B-type stars as dictated by stellar evolution. Here I extend this research to the Local Group galaxies M31 and M33 and investigate the RSG binary fraction as…

2021 The Astrophysical Journal
eHST 29
The Age of Westerlund 1 Revisited
DOI: 10.3847/1538-4357/abec44 Bibcode: 2021ApJ...912...16B

Smith, Nathan; Gehrz, Robert D.; Figer, Donald F. +2 more

The cluster Westerlund 1 (Wd1) is host to a large variety of post-main-sequence (MS) massive stars. The simultaneous presence of these stars can only be explained by stellar models if the cluster has a finely tuned age of 4-5 Myr, with several published studies independently claiming ages within this range. At this age, stellar models predict that…

2021 The Astrophysical Journal
Gaia 29
Distant Relatives: The Chemical Homogeneity of Comoving Pairs Identified in Gaia
DOI: 10.3847/1538-4357/ac14be Bibcode: 2021ApJ...921..118N

Ting, Yuan-Sen; Hawkins, Keith; El-Badry, Kareem +3 more

Comoving pairs, even at the separations of ${ \mathcal O }({10}^{6})$ au, are a predicted reservoir of conatal stars. We present detailed chemical abundances of 62 stars in 31 comoving pairs with separations of 102-107 au and 3D velocity differences <2 km s-1. This sample includes both bound comoving pairs/wide …

2021 The Astrophysical Journal
Gaia 29
NGC 5128 Globular Cluster Candidates Out to 150 kpc: A Comprehensive Catalog from Gaia and Ground-based Data
DOI: 10.3847/1538-4357/abf63c Bibcode: 2021ApJ...914...16H

Forbes, Duncan A.; Caldwell, Nelson; Strader, Jay +9 more

We present a new catalog of 40,502 globular cluster (GC) candidates in NGC 5128 out to a projected radius of ~150 kpc based on data from the Panoramic Imaging Survey of Centaurus and Sculptor, the Gaia Data Release 2, and the NOAO Source Catalog. Ranking these candidates based on the likelihood that they are true GCs, we find that approximately 19…

2021 The Astrophysical Journal
Gaia 29
Observations of Magnetic Fields Surrounding LkHα 101 Taken by the BISTRO Survey with JCMT-POL-2
DOI: 10.3847/1538-4357/abd0fc Bibcode: 2021ApJ...908...10N

Zhang, Yapeng; Pattle, Kate; Ward-Thompson, Derek +146 more

We report the first high spatial resolution measurement of magnetic fields surrounding LkHα 101, part of the Auriga-California molecular cloud. The observations were taken with the POL-2 polarimeter on the James Clerk Maxwell Telescope within the framework of the B-fields In Star-forming Region Observations (BISTRO) survey. Observed polarization o…

2021 The Astrophysical Journal
Gaia Herschel 29
Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters
DOI: 10.3847/1538-4357/ac2578 Bibcode: 2021ApJ...922..114S

Pérez-González, Pablo G.; Koekemoer, Anton M.; Smail, Ian +22 more

We present a Spitzer/IRAC survey of H-faint (H 160 ≳ 26.4, < 5σ) sources in 101 lensing cluster fields. Across a CANDELS/Wide-like survey area of ~648 arcmin2 (effectively ~221 arcmin2 in the source plane), we have securely discovered 53 sources in the IRAC Channel-2 band (CH2, 4.5 µm; median CH2 = 22.46 ±…

2021 The Astrophysical Journal
Gaia Herschel eHST 29
Detection of Flare Multiperiodic Pulsations in Mid-ultraviolet Balmer Continuum, Lyα, Hard X-Ray, and Radio Emissions Simultaneously
DOI: 10.3847/1538-4357/ac1c05 Bibcode: 2021ApJ...921..179L

Li, Gang; Gan, Weiqun; Li, Xiaobo +7 more

Quasi-periodic pulsations (QPPs), which usually appear as temporal pulsations of the total flux, are frequently detected in the light curves of solar/stellar flares. In this study, we present the investigation of nonstationary QPPs with multiple periods during the impulsive phase of a powerful flare on 2017 September 6, which were simultaneously m…

2021 The Astrophysical Journal
PROBA-2 29
Testing Evolutionary Models with Red Supergiant and Wolf-Rayet Populations
DOI: 10.3847/1538-4357/ac15f5 Bibcode: 2021ApJ...922..177M

Massey, Philip; Dorn-Wallenstein, Trevor Z.; Levesque, Emily M. +3 more

Despite the many successes that modern massive star evolutionary theory has enjoyed, reproducing the apparent trend in the relative number of red supergiants (RSGs) and Wolf-Rayet (WR) stars has remained elusive. Previous estimates show the RSG/WR ratio decreasing strongly with increasing metallicity. However, the evolutionary models have always p…

2021 The Astrophysical Journal
Gaia 29