Search Publications

The orbital phase space of contracted dark matter haloes
DOI: 10.1093/mnras/staa1089 Bibcode: 2020MNRAS.495...12C

Grand, Robert J. J.; Marinacci, Federico; Deason, Alis J. +4 more

We study the orbital phase space of dark matter (DM) haloes in the AURIGA suite of cosmological hydrodynamics simulations of Milky Way (MW) analogues. We characterize haloes by their spherical action distribution, $F\left(J_{{r}},L\right)$ , a function of the specific angular momentum, L, and the radial action, Jr, of the DM particles. …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 24
Formation pathway for lonely stripped-envelope supernova progenitors: implications for Cassiopeia A
DOI: 10.1093/mnras/staa2898 Bibcode: 2020MNRAS.499.1154H

Sato, Toshiki; Podsiadlowski, Philipp; Mandel, Ilya +2 more

We explore a new scenario for producing stripped-envelope supernova progenitors. In our scenario, the stripped-envelope supernova is the second supernova of the binary, in which the envelope of the secondary was removed during its red supergiant phase by the impact of the first supernova. Through 2D hydrodynamical simulations, we find that ∼50-90 …

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 24
Efficient Methanol Production on the Dark Side of a Prestellar Core
DOI: 10.3847/1538-4357/ab8f93 Bibcode: 2020ApJ...895..101H

Bizzocchi, Luca; Caselli, Paola; Rosolowsky, Erik +23 more

We present Atacama Large Millimeter/submillimeter Array maps of the starless molecular cloud core Ophiuchus/H-MM1 in the lines of deuterated ammonia (ortho- ${\mathrm{NH}}_{2}{\rm{D}}$ ), methanol ( ${\mathrm{CH}}_{3}\mathrm{OH}$ ), and sulfur monoxide (SO). The dense core is seen in ${\mathrm{NH}}_{2}{\rm{D}}$ emission, whereas the ${\mathrm{CH}}…

2020 The Astrophysical Journal
Herschel 24
A catalogue of over 10 million variable source candidates in ZTF Data Release 1
DOI: 10.1093/mnras/staa2814 Bibcode: 2020MNRAS.499.5782O

Gal-Yam, Avishay; Ofek, Eran O.; Masci, Frank +4 more

Variable sources probe a wide range of astrophysical phenomena. We present a catalogue of over 10 million variable source candidates found in Data Release 1 (DR1) of the Zwicky Transient Facility (ZTF). We perform a periodicity search up to a frequency of 160 d-1, and we classify the light curves into erratic and smooth variables. We al…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 24
LAMOST Observations in 15 K2 Campaigns. I. Low-resolution Spectra from LAMOST DR6
DOI: 10.3847/1538-4365/abc1ed Bibcode: 2020ApJS..251...27W

Shi, Jianrong; Zong, Weikai; Fu, Jian-Ning +12 more

The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST)-K2 (LK2) project, initiated in 2015, aims to collect low-resolution spectra of targets in the K2 campaigns, similar to the LAMOST-Kepler project. By the end of 2018, a total of 126 LK2 plates had been observed by LAMOST. After cross-matching the catalog of the LAMOST data relea…

2020 The Astrophysical Journal Supplement Series
Gaia 24
Estimating the size of X-ray lamppost coronae in active galactic nuclei
DOI: 10.1051/0004-6361/202039158 Bibcode: 2020A&A...644A.132U

Done, C.; Petrucci, P. -O.; Matt, G. +3 more


Aims: We report estimates of the X-ray coronal size of active galactic nuclei in the lamppost geometry. In this commonly adopted scenario, the corona is assumed for simplicity to be a point-like X-ray source located on the axis of the accretion disc. However, the corona must intercept a number of optical/UV seed photons from the disc consiste…

2020 Astronomy and Astrophysics
XMM-Newton 24
MOSEL: Strong [OIII] 5007 Å Emitting Galaxies at (3 < z < 4) from the ZFOURGE Survey
DOI: 10.3847/1538-4357/ab8cba Bibcode: 2020ApJ...898...45T

Papovich, Casey; Kacprzak, Glenn G.; Glazebrook, Karl +13 more

To understand how strong emission-line galaxies (SELGs) contribute to the overall growth of galaxies and star formation history of the universe, we target SELGs from the ZFOURGE imaging survey that have blended Hβ+[O III] rest-frame equivalent widths of >230 Å and 2.5 < ${z}_{\mathrm{phot}}$ < 4.0. Using Keck/MOSFIRE, we measure 49 redshi…

2020 The Astrophysical Journal
Herschel eHST 23
Zodiacal exoplanets in time - XI. The orbit and radiation environment of the young M dwarf-hosted planet K2-25b
DOI: 10.1093/mnrasl/slaa136 Bibcode: 2020MNRAS.498L.119G

Kuzuhara, M.; Tamura, M.; Kudo, T. +20 more

M dwarf stars are high-priority targets for searches for Earth-size and potentially Earth-like planets, but their planetary systems may form and evolve in very different circumstellar environments than those of solar-type stars. To explore the evolution of these systems, we obtained transit spectroscopy and photometry of the Neptune-size planet or…

2020 Monthly Notices of the Royal Astronomical Society
eHST 23
Possible ∼0.4 h X-ray quasi-periodicity from an ultrasoft active galactic nucleus
DOI: 10.1051/0004-6361/202039410 Bibcode: 2020A&A...644L...9S

Xue, Y. Q.; Shu, X. W.; Wang, T. G. +6 more

RX J1301.9+2747 is an ultrasoft active galactic nucleus (AGN) with unusual X-ray variability that is characterized by a long quiescent state and a short-lived flare state. The X-ray flares are found to recur quasi-periodically on a timescale of 13-20 ks. Here, we report the analysis of the light curve in the quiescent state from two XMM-Newton obs…

2020 Astronomy and Astrophysics
XMM-Newton 23
The Blue Compact Dwarf Galaxy VCC 848 Formed by Dwarf-Dwarf Merging: H I Gas, Star Formation, and Numerical Simulations
DOI: 10.3847/1538-4357/abab96 Bibcode: 2020ApJ...900..152Z

Gao, Yu; Rong, Yu; Hunter, Deidre A. +12 more

A clear link between a dwarf-dwarf merger event and enhanced star formation (SF) in the recent past was recently identified in the gas-dominated merger remnant VCC 848, offering by far the clearest view of a gas-rich late-stage dwarf-dwarf merger. We present a joint analysis of JVLA H I emission line mapping, optical imaging, and numerical simulat…

2020 The Astrophysical Journal
Herschel 23