Search Publications

Possible Time Correlation between Jet Ejection and Mass Accretion for RW Aur A
DOI: 10.3847/1538-4357/abab98 Bibcode: 2020ApJ...901...24T

Ohyama, Youichi; Pyo, Tae-Soo; Liu, Chun-Fan +17 more

For the active T-Taur star RW Aur A we have performed long-term (∼10 yr) monitoring observations of (1) jet imaging in the [Fe II] 1.644 µm emission line using Gemini-NIFS and VLT-SINFONI; (2) optical high-resolution spectroscopy using CFHT-ESPaDOnS; and (3) V-band photometry using the CrAO 1.25-m telescope and AAVSO. The latter two observat…

2020 The Astrophysical Journal
Gaia 13
On the X-Ray Spectral Energy Distributions of Star-forming Galaxies: The 0.3-30 keV Spectrum of the Low-metallicity Starburst Galaxy VV 114
DOI: 10.3847/1538-4357/abba2d Bibcode: 2020ApJ...903...79G

Hornschemeier, Ann; Basu-Zych, Antara; Garofali, Kristen +6 more

Binary population synthesis combined with cosmological models suggests that X-ray emission from star-forming galaxies, consisting primarily of emission from X-ray binaries (XRBs) and the hot interstellar medium (ISM), could be an important, and perhaps dominant, source of heating of the intergalactic medium prior to the epoch of reionization. Howe…

2020 The Astrophysical Journal
XMM-Newton eHST 13
Relation of Coronal Rain Originating from Coronal Condensations to Interchange Magnetic Reconnection
DOI: 10.3847/1538-4357/abc68c Bibcode: 2020ApJ...905...26L

Peter, Hardi; Li, Leping; Chitta, Lakshmi Pradeep +1 more

Using extreme-ultraviolet images, we recently proposed a new and alternative formation mechanism for coronal rain along magnetically open field lines due to interchange magnetic reconnection. In this paper we report coronal rain at chromospheric and transition region temperatures originating from the coronal condensations facilitated by reconnecti…

2020 The Astrophysical Journal
IRIS 13
Discovery of Tidal Tails around the Old Open Cluster NGC 2506
DOI: 10.3847/1538-4357/ab8560 Bibcode: 2020ApJ...894...48G

Gao, Xinhua

We report the discovery of tidal tails around the old open cluster NGC 2506 based on Gaia-DR2. A principal-component analysis and Gaussian mixture model are used to identify extra-tidal stars. We identify 2301 stars closely related to the cluster, 147 of which are likely extra-tidal stars. We find clear evidence for the existence of two well-defin…

2020 The Astrophysical Journal
Gaia 13
Eclipsing Binaries in the Open Cluster Ruprecht 147. III. The Triple System EPIC 219552514 at the Main-sequence Turnoff
DOI: 10.3847/1538-4357/ab911b Bibcode: 2020ApJ...896..162T

Torres, Guillermo; Vanderburg, Andrew; Rizzuto, Aaron C. +3 more

Spectroscopic observations are reported for the 2.75 day, double-lined, detached eclipsing binary EPIC 219552514 located at the turnoff of the old nearby open cluster Ruprecht 147. A joint analysis of our radial-velocity measurements and the K2 light curve leads to masses of ${M}_{1}={1.509}_{-0.056}^{+0.063}\,{M}_{\odot }$ and ${M}_{2}={0.649}_{-…

2020 The Astrophysical Journal
Gaia 13
OGLE-ing the Magellanic System: Cepheids in the Bridge
DOI: 10.3847/1538-4357/ab61f1 Bibcode: 2020ApJ...889...25J

Udalski, Andrzej; Mróz, Przemek; Szymański, Michał K. +12 more

We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimension…

2020 The Astrophysical Journal
Gaia 13
Measuring the Heating and Cooling of the Interstellar Medium at High Redshift: PAH and [C II] Observations of the Same Star-forming Galaxies at z ∼ 2
DOI: 10.3847/1538-4357/ab77b9 Bibcode: 2020ApJ...892..119M

Kirkpatrick, Allison; Dickinson, Mark E.; McKinney, Jed +4 more

Star formation depends critically on cooling mechanisms in the interstellar medium (ISM); however, thermal properties of gas in galaxies at the peak epoch of star formation (z ∼ 2) remain poorly understood. A limiting factor in understanding the multiphase ISM is the lack of multiple tracers detected in the same galaxies, such as Polycyclic Aromat…

2020 The Astrophysical Journal
Herschel eHST 13
On the Absence of High-redshift AGNs: Little Growth in the Supermassive Black Hole Population at High Redshifts
DOI: 10.3847/1538-4357/ab6aaa Bibcode: 2020ApJ...891...69C

Bauer, F. E.; Barger, A. J.; Cowie, L. L. +1 more

We search for high-redshift (z > 4.5) X-ray active galactic nuclei (AGNs) in the deep central (off-axis angle < 5'7) region of the 7 Ms Chandra Deep Field-South X-ray image. We compile an initial candidate sample from direct X-ray detections. We then probe more deeply in the X-ray data by using preselected samples with high spatial resolutio…

2020 The Astrophysical Journal
eHST 13
A Magnetic White Dwarf Accretion Model for the Anomalous X-Ray Pulsar 4U 0142+61
DOI: 10.3847/1538-4357/ab8add Bibcode: 2020ApJ...895...26B

Rodrigues, Claudia V.; Coelho, Jaziel G.; Castro, Manuel +2 more

The quiescent emission of the anomalous X-ray pulsar (AXP) 4U 0142+61 extends over a broad range of energy, from radio up to hard X-rays. In particular, this object is unique among soft gamma-ray repeaters (SGRs) and AXPs in presenting simultaneously mid-infrared emission and pulsed optical emission. In spite of the many propositions to explain th…

2020 The Astrophysical Journal
INTEGRAL 12
The Demagnetization of the Venusian Ionosphere under Nearly Flow-aligned Interplanetary Magnetic Fields
DOI: 10.3847/1538-4357/aba62a Bibcode: 2020ApJ...900...63C

Xu, Qi; Zhang, Tielong; Xu, Xiaojun +4 more

Previous studies suggested that the interplanetary magnetic field (IMF) has a significant influence on the Venusian-induced magnetosphere. We present observations by Venus Express under a nearly flow-aligned IMF condition to investigate the demagnetization of the Venusian ionosphere. Our results show that the magnetic barrier becomes weak and narr…

2020 The Astrophysical Journal
VenusExpress 12