Search Publications

A Broadband Look at the Old and New ULXs of NGC 6946
DOI: 10.3847/1538-4357/ab20cd Bibcode: 2019ApJ...881...38E

Fürst, Felix; Walton, Dominic J.; Stern, Daniel +8 more

Two recent observations of the nearby galaxy NGC 6946 with NuSTAR, one simultaneous with an XMM-Newton observation, provide an opportunity to examine its population of bright accreting sources from a broadband perspective. We study the three known ultraluminous X-ray sources (ULXs) in the galaxy, and find that ULX-1 and ULX-2 have very steep power…

2019 The Astrophysical Journal
XMM-Newton eHST 20
Isochrone-cloud fitting of the extended main-sequence turn-off of young clusters
DOI: 10.1051/0004-6361/201936549 Bibcode: 2019A&A...632A..74J

Bastian, N.; Aerts, C.; Johnston, C. +1 more

Context. Extended main-sequence turn-offs (eMSTOs) are a commonly observed property of young clusters. A global theoretical interpretation for eMSTOs is still lacking, but stellar rotation is considered a necessary ingredient to explain eMSTOs.
Aims: We aim to assess the importance of core-boundary and envelope mixing in stellar interiors for…

2019 Astronomy and Astrophysics
eHST 20
VLT/SPHERE Multiwavelength High-contrast Imaging of the HD 115600 Debris Disk: New Constraints on the Dust Geometry and the Presence of Young Giant Planets
DOI: 10.3847/1538-3881/aaf1bd Bibcode: 2019AJ....157...39G

Currie, Thayne; Wagner, Kevin; Moór, Attila +5 more

Young and dynamically active planetary systems can form disks of debris that are easier to image than the planets themselves. The morphology and evolution of these disks can help to infer the properties of the putative planets responsible for generating and shaping the debris structures. We present integral field spectroscopy and dual-band imaging…

2019 The Astronomical Journal
Gaia Herschel 20
Testing the Kerr Metric with X-Ray Reflection Spectroscopy of Mrk 335 Suzaku Data
DOI: 10.3847/1538-4357/ab24d6 Bibcode: 2019ApJ...879...80C

Abdikamalov, Askar B.; Ayzenberg, Dimitry; Bambi, Cosimo +4 more

Einstein’s gravity has undergone extensive tests in the weak field gravitational limit, with results in agreement with theoretical predictions. There exist theories beyond general relativity (GR) which modify gravity in the strong field regime but agree with GR in the weak field. Astrophysical black holes are believed to be described by the Kerr m…

2019 The Astrophysical Journal
Suzaku XMM-Newton 20
Statistics on the Magnetosheath Properties Related to Magnetopause Magnetic Reconnection
DOI: 10.3847/1538-4357/ab290e Bibcode: 2019ApJ...880..122Z

Zhang, Hui; Liu, Libo; Wan, Weixing +5 more

Magnetosheath properties, particularly those related to magnetopause magnetic reconnection (MR), are investigated in this study. (1) Asymmetries are found to exist in the distributions of plasma and magnetic field parameters in the magnetosheath. These asymmetries are related to the interplanetary magnetic field (IMF) orientation, and they are pro…

2019 The Astrophysical Journal
Cluster 20
Searching for Black Hole Candidates by LAMOST and ASAS-SN
DOI: 10.3847/1538-3881/ab449f Bibcode: 2019AJ....158..179Z

Liu, Jifeng; Bai, Yu; Gu, Wei-Min +13 more

Most dynamically confirmed stellar-mass black holes (BHs) and their candidates were originally selected from X-ray outbursts. In the present work, we search for BH candidates in the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) survey using the spectra along with photometry from the All Sky Automated Survey for SuperNovae (ASA…

2019 The Astronomical Journal
Gaia 20
Extended X-Ray Study of M49: The Frontier of the Virgo Cluster
DOI: 10.3847/1538-3881/ab1d51 Bibcode: 2019AJ....158....6S

Mernier, F.; Churazov, E.; Maccarone, T. J. +10 more

The M49 group, residing outside the virial radius of the Virgo cluster, is falling onto the cluster from the south. We report results from deep XMM-Newton mosaic observations of M49. Its hot gas temperature is 0.8 keV at the group center and rises to 1.5 keV beyond the brightest group galaxy (BGG). The group gas extends to radii of ∼300 kpc to the…

2019 The Astronomical Journal
XMM-Newton 20
The Herschel-PACS North Ecliptic Pole Survey
DOI: 10.1093/pasj/psy107 Bibcode: 2019PASJ...71...13P

Goto, Tomotsugu; Kim, Seong Jin; Pearson, Chris +9 more

A detailed analysis of Herschel/Photoconductor Array Camera and Spectrometer (PACS) observations at the North Ecliptic Pole is presented. High-quality maps, covering an area of 0.44 deg2, are produced and then used to derive potential candidate source lists. A rigorous quality-control pipeline has been used to create final legacy catalo…

2019 Publications of the Astronomical Society of Japan
AKARI Herschel 20
The complex evolution of the X-ray binary transient MAXI J1807+132 along the decay of its discovery outburst
DOI: 10.1093/mnras/sty3457 Bibcode: 2019MNRAS.484.2078J

Russell, D. M.; Armas Padilla, M.; Jiménez-Ibarra, F. +6 more

MAXI J1807+132 is an X-ray transient discovered during the decay of an outburst in 2017. We present optical and X-ray monitoring of the source over more than 125 d, from outburst to quiescence. The outburst decay is characterized by the presence of several reflares with a quasi-periodic recurrence time of ∼6.5 d. We detect broad H and He emission …

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 20
Wide-area photometric and astrometric (Gaia DR2) study of the young cluster NGC 6530
DOI: 10.1051/0004-6361/201833877 Bibcode: 2019A&A...623A..25D

Micela, G.; Sciortino, S.; Prisinzano, L. +1 more

Context. NGC 6530 is a young cluster, with a complex morphology and star-formation history. We present a statistical study of its global properties, using a new, large list of candidate members down to masses of 0.2-0.4 M and Gaia DR2 astrometry.
Aims: We consider a larger sky region compared to previous studies, to investigate th…

2019 Astronomy and Astrophysics
Gaia 20