Search Publications

X-ray reverberation lags of the Fe-K line due to AGN disc winds
DOI: 10.1093/mnras/sty3056 Bibcode: 2019MNRAS.482.5316M

Done, Chris; Tsujimoto, Masahiro; Ebisawa, Ken +3 more

Short X-ray reverberation lags are seen across a broad Fe-K energy band in more than 20 active galactic nuclei (AGNs). This broad iron line feature in the lag spectrum is most significant in super-Eddington sources such as Ark 564 (L/LEdd ∼ 1) and 1H 0707-495 (L/LEdd ≳ 10). The observed lag time-scales correspond to very shor…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 21
The long outburst of the black hole transient GRS 1716-249 observed in the X-ray and radio band
DOI: 10.1093/mnras/sty2739 Bibcode: 2019MNRAS.482.1587B

Motta, S. E.; Segreto, A.; Malzac, J. +9 more

We present the spectral and timing analysis of X-ray observations performed on the Galactic black hole transient GRS 1716-249 during the 2016-2017 outburst. The source was almost continuously observed with the Neil Gehrels Swift Observatory from 2016 December until 2017 October. The X-ray hardness ratio and timing evolution indicate that the sourc…

2019 Monthly Notices of the Royal Astronomical Society
INTEGRAL 21
Coordinates and Maps of the Apollo 17 Landing Site
DOI: 10.1029/2018EA000408 Bibcode: 2019E&SS....6...59H

Oberst, Jürgen; Haase, Isabel; Wählisch, Marita +2 more

We carried out an extensive cartographic analysis of the Apollo 17 landing site and determined and mapped positions of the astronauts, their equipment, and lunar landmarks with accuracies of better than ±1 m in most cases. To determine coordinates in a lunar body-fixed coordinate frame, we applied least squares (2-D) network adjustments to angular…

2019 Earth and Space Science
MEx 21
Isochronal age-mass discrepancy of young stars: SCExAO/CHARIS integral field spectroscopy of the HIP 79124 triple system
DOI: 10.1051/0004-6361/201834688 Bibcode: 2019A&A...622A..42A

Henning, Thomas; Nakagawa, Takao; Currie, Thayne +24 more

We present SCExAO/CHARIS 1.1-2.4 µm integral field direct spectroscopy of the young HIP 79124 triple system. HIP 79124 is a member of the Scorpius-Centaurus association, consisting of an A0V primary with two low-mass companions at a projected separation of < 1″. Thanks to the high quality wavefront corrections provided by SCExAO, both com…

2019 Astronomy and Astrophysics
Gaia 21
Two Jovian Planets around the Giant Star HD 202696: A Growing Population of Packed Massive Planetary Pairs around Massive Stars?
DOI: 10.3847/1538-3881/aafa11 Bibcode: 2019AJ....157...93T

Trifonov, Trifon; Stock, Stephan; Henning, Thomas +6 more

We present evidence for a new two-planet system around the giant star HD 202696 (=HIP 105056, BD +26 4118). The discovery is based on public HIRES radial velocity (RV) measurements taken at Keck Observatory between 2007 July and 2014 September. We estimate a stellar mass of {1.91}-0.14+0.09{M} for HD 202696, whic…

2019 The Astronomical Journal
Gaia Hipparcos 21
Global Parameters of 12 Totally Eclipsing W UMa Stars
DOI: 10.3847/1538-3881/ab4203 Bibcode: 2019AJ....158..186K

Popov, Velimir A.; Petrov, Nikola I.; Kjurkchieva, Diana P.

Photometric observations of 12 totally eclipsing W UMa binaries (NSVS 3325547, V646 Lac, V1320 Cas, V539 Dra, V816 Cep, NSVS 9045055, V1115 Cas, V902 Cep, V596 Peg, NSVS 1768818, V619 Peg, and NSVS 3198272) are presented. We found that the longer (in phase units) the flat eclipses are, the smaller the mass ratios (or the reciprocal values) are. Th…

2019 The Astronomical Journal
Gaia 21
TESS Habitable Zone Star Catalog
DOI: 10.3847/2041-8213/ab0e8d Bibcode: 2019ApJ...874L...8K

Stassun, K.; Kaltenegger, L.; Pepper, J. +1 more

We present the Transiting Exoplanet Survey Satellite (TESS) Habitable Zone Stars Catalog, a list of 1822 nearby stars with a TESS magnitude brighter than T = 12 and reliable distances from Gaia DR2, around which the NASA’s TESS mission can detect transiting planets, which receive Earth-like irradiation. For all those stars TESS is sensitive down t…

2019 The Astrophysical Journal
Gaia 21
The chemistry of stars in the bar of the Milky Way
DOI: 10.1051/0004-6361/201936779 Bibcode: 2019A&A...632A.121W

Schultheis, M.; Rojas-Arriagada, A.; Wegg, C. +1 more

We use a sample of 938 red clump giant stars located in the direction of the Galactic long bar to study the chemistry of Milky Way bar stars. Kinematically separating stars on bar orbits from stars with inner disc orbits, we find that stars on bar-like orbits are more metal rich with a mean iron abundance of ⟨[Fe/H]⟩ = +0.30 compared to ⟨[Fe/H]⟩ =…

2019 Astronomy and Astrophysics
Gaia 21
Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2≲ z ≲0.9
DOI: 10.1093/mnras/sty3335 Bibcode: 2019MNRAS.485..586R

Rodighiero, G.; Valtchanov, I.; Franceschini, A. +21 more

We quantify the star formation (SF) in the inner cores (R/R200 ≤0.3) of 24 massive galaxy clusters at 0.2≲ z ≲0.9 observed by the Herschel Lensing Survey and the Cluster Lensing and Supernova survey with Hubble. These programmes, covering the rest-frame ultraviolet to far-infrared regimes, allow us to accurately characterize stellar mas…

2019 Monthly Notices of the Royal Astronomical Society
Herschel eHST 21
Masses, oxygen, and carbon abundances in CHEPS dwarf stars
DOI: 10.1051/0004-6361/201834138 Bibcode: 2019A&A...621A.112P

Jones, H. R. A.; Jenkins, J. S.; Pavlenko, Y. V. +3 more

Context. We report the results from the determination of stellar masses, carbon, and oxygen abundances in the atmospheres of 107 stars from the Calan-Hertfordshire Extrasolar Planet Search (CHEPS) programme. Our stars are drawn from a population with a significantly super-solar metallicity. At least 10 of these stars are known to host orbiting pla…

2019 Astronomy and Astrophysics
Gaia 21