Search Publications

Correction to the Photometric Colors of Gaia Early Data Release 3
DOI: 10.3847/2041-8213/abe1c2 Bibcode: 2021ApJ...908L..14N

Niu, Zexi; Liu, Jifeng; Yuan, Haibo

In this work, we use the spectroscopy-based stellar color regression method with ∼0.7 million common stars between LAMOST DR7 and Gaia EDR3 to acquire color corrections in G - GRP and GBP - GRP. A sub-millimagnitude precision is achieved. Our results demonstrate that improvements in the calibration process of the E…

2021 The Astrophysical Journal
Gaia 22
Spiral Arm Pattern Motion in the SAO 206462 Protoplanetary Disk
DOI: 10.3847/2041-8213/abd241 Bibcode: 2021ApJ...906L...9X

Dong, Ruobing; Pueyo, Laurent; Stolker, Tomas +5 more

Spiral arms have been observed in more than a dozen protoplanetary disks, yet the origin of nearly all systems is under debate. Multi-epoch monitoring of spiral arm morphology offers a dynamical way to distinguish two leading arm formation mechanisms: companion-driven and gravitational instability induction, since these mechanisms predict distinct…

2021 The Astrophysical Journal
Gaia 22
Multiple Stellar Populations in Asymptotic Giant Branch Stars of Galactic Globular Clusters
DOI: 10.3847/1538-4357/abdfcf Bibcode: 2021ApJ...910....6L

Milone, A. P.; Cordoni, G.; Marino, A. F. +8 more

Multiple stellar populations (MPs) are a distinct characteristic of globular clusters (GCs). Their general properties have been widely studied among main-sequence, red giant branch (RGB), and horizontal branch (HB) stars, but a common framework is still missing at later evolutionary stages. We studied the MP phenomenon along the asymptotic giant b…

2021 The Astrophysical Journal
eHST 22
The Late-time Radio Behavior of Gamma-ray Burst Afterglows: Testing the Standard Model
DOI: 10.3847/1538-4357/abe76b Bibcode: 2021ApJ...911...14K

Fruchter, Andrew S.; Kangas, Tuomas

We examine a sample of 21 gamma-ray burst (GRB) afterglow light curves at radio frequencies and compare them to the X-ray and/or optical properties of the afterglows and to the predictions of the standard jet/fireball model. Our sample includes every Swift GRB with an X-ray light curve indicating a jet break and with a published radio light curve,…

2021 The Astrophysical Journal
eHST 22
A Near-infrared Survey of UV-excited Molecular Hydrogen in Photodissociation Regions
DOI: 10.3847/1538-4357/ac0899 Bibcode: 2021ApJ...919...27K

Kim, Hwihyun; Dinerstein, Harriet L.; Jaffe, Daniel T. +1 more

We present a comparative study of the near-infrared (NIR) H2 line emission from five regions near hot young stars: Sharpless 140, NGC 2023, IC 63, the Horsehead Nebula, and the Orion Bar. This emission originates in photodissociation or photon-dominated regions (PDRs), interfaces between photoionized and molecular gas near hot (O) stars…

2021 The Astrophysical Journal
Gaia 22
The Be Star 66 Ophiuchi: 60 Years of Disk Evolution
DOI: 10.3847/1538-4357/abed4c Bibcode: 2021ApJ...912...76M

Carciofi, A. C.; Mota, B. C.; Jones, C. E. +5 more

We use a time-dependent hydrodynamic code and a non-LTE Monte Carlo code to model disk dissipation for the Be star 66 Ophiuchi. We compiled 63 years of observations from 1957 to 2020 to encompass the complete history of the growth and subsequent dissipation of the star's disk. Our models are constrained by new and archival photometry, spectroscopy…

2021 The Astrophysical Journal
AKARI Gaia IUE 22
Caltech-NRAO Stripe 82 Survey (CNSS). V. AGNs That Transitioned to Radio-loud State
DOI: 10.3847/1538-4357/abe62d Bibcode: 2021ApJ...914...22W

Gromadzki, Mariusz; Hallinan, Gregg; Ishwara-Chandra, C. H. +6 more

A recent multiyear Caltech-NRAO Stripe 82 Survey revealed a group of objects that appeared as new radio sources after >5-20 yr of absence. They are transient phenomena with respect to the Faint Images of the Radio Sky at Twenty Centimeters survey and constitute the first unbiased sample of renewed radio activity. Here we present a follow-up, ra…

2021 The Astrophysical Journal
XMM-Newton 22
Hybrid Comptonization and Electron-Positron Pair Production in the Black-hole X-Ray Binary MAXI J1820+070
DOI: 10.3847/2041-8213/ac0147 Bibcode: 2021ApJ...914L...5Z

Poutanen, Juri; Zdziarski, Andrzej A.; Szanecki, Michał +6 more

We study X-ray and soft gamma-ray spectra from the hard state of the accreting black-hole binary MAXI J1820+070. We perform an analysis of two joint spectra from NuSTAR and INTEGRAL, covering the range of 3-650 keV, and of an average joint spectrum over the rise of the hard state, covering the 3-2200 keV range. The spectra are well modeled by Comp…

2021 The Astrophysical Journal
INTEGRAL 22
Dynamical Analysis of the Dark Matter and Central Black Hole Mass in the Dwarf Spheroidal Leo I
DOI: 10.3847/1538-4357/ac0c79 Bibcode: 2021ApJ...921..107B

Gebhardt, Karl; Zeimann, Greg; Thomas, Jens +4 more

We measure the central kinematics for the dwarf spheroidal galaxy Leo I using integrated-light measurements and previously published data. We find a steady rise in the velocity dispersion from 300″ into the center. The integrated-light kinematics provide a velocity dispersion of 11.76 ± 0.66 km s-1 inside 75″. After applying appropriate…

2021 The Astrophysical Journal
eHST 22
A Blueprint for the Milky Way's Stellar Populations. III. Spatial Distributions and Population Fractions of Local Halo Stars
DOI: 10.3847/1538-4357/ac07a4 Bibcode: 2021ApJ...918...74A

Beers, Timothy C.; An, Deokkeun

We analyze the observed spatial, chemical and dynamical distributions of local metal-poor stars, based on photometrically derived metallicity and distance estimates along with proper motions from the Gaia mission. Along the Galactic prime meridian, we identify stellar populations with distinct properties in the metallicity versus rotational veloci…

2021 The Astrophysical Journal
Gaia 22