Search Publications

Keck HIRES spectroscopy of SkyMapper commissioning survey candidate extremely metal-poor stars
DOI: 10.1093/mnras/stz645 Bibcode: 2019MNRAS.485.5153M

Schmidt, B. P.; Da Costa, G. S.; Marino, A. F. +11 more

We present results from the analysis of high-resolution spectra obtained with the Keck HIRES spectrograph for a sample of 17 candidate extremely metal-poor (EMP) stars originally selected from commissioning data obtained with the SkyMapper telescope. Fourteen of the stars have not been observed previously at high dispersion. Three have [Fe/H] ≤ -3…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 12
Anomalous behaviour of the UV-optical continuum bands in NGC 5548
DOI: 10.1093/mnras/stz1186 Bibcode: 2019MNRAS.486.5362G

Knigge, C.; Kriss, G. A.; Starkey, D. A. +8 more

During the 2014 HST/Swift and ground-based multiwavelength monitoring campaign of NGC 5548 [active galactic nucleus (AGN) STORM], the UV-optical broad emission lines exhibited anomalous, decorrelated behaviour relative to the far-UV continuum flux variability. Here, we use key diagnostic emission lines (Ly α and He II) for this campaign to infer a…

2019 Monthly Notices of the Royal Astronomical Society
eHST 12
An all-sky search for R Coronae Borealis stars in ASAS-SN
DOI: 10.1093/mnras/sty3445 Bibcode: 2019MNRAS.483.4470S

Kochanek, C. S.; Stanek, K. Z.; Dong, Subo +6 more

We report the discovery of 19 new R Coronae Borealis (RCB) star and DY Per candidates with light curves from the All-Sky Automated Survey for Supernovae. We examined both an existing set of 1602 near/mid-infrared (IR) selected candidates and an additional 2615 candidates selected to have near/mid-IR spectral energy distributions consistent with th…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 12
The morpho-kinematics of the circumstellar envelope around the AGB star EP Aqr
DOI: 10.1093/mnras/stz041 Bibcode: 2019MNRAS.484.1865H

Winters, J. M.; Tuan-Anh, P.; Hoai, D. T. +6 more

ALMA observations of CO(1-0) and CO(2-1) emissions of the circumstellar envelope of EP Aqr, an oxygen-rich asymptotic giant branch star, are reported. A thorough analysis of their properties is presented using an original method based on the separation of the data cube into a low-velocity component associated with an equatorial outflow and a faste…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 12
Modelling the abundance structure of isocyanic acid (HNCO) towards the low-mass solar type protostar IRAS 16293-2422
DOI: 10.1093/mnras/sty2971 Bibcode: 2019MNRAS.483.2014H

Menten, Karl M.; Loinard, Laurent; Wiesenfeld, Laurent +5 more

Isocyanic acid (HNCO), the most stable of the simplest molecules containing the four main elements essential for organic chemistry, has been observed in several astrophysical environments such as molecular clouds, star-forming regions, external galaxies, and comets. In this work, we model HNCO spectral line profiles towards the low-mass solar type…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 12
Beyond the Minisolar Maximum of Solar Cycle 24: Declining Solar Magnetic Fields and the Response of the Terrestrial Magnetosphere
DOI: 10.1029/2019JA026616 Bibcode: 2019JGRA..124.6363I

Janardhan, P.; Ingale, M.; Bisoi, S. K.

The present study examines the response of the terrestrial magnetosphere to the long-term steady declining trends observed in solar magnetic fields and solar wind microturbulence levels since mid-1990s that has been continuing beyond the minisolar maximum of cycle 24. A detailed analysis of the response of the terrestrial magnetosphere has been ca…

2019 Journal of Geophysical Research (Space Physics)
Cluster 12
UV to X-Ray Comptonization Delay in Mrk 493
DOI: 10.3847/2041-8213/aaf8ab Bibcode: 2019ApJ...870L..13A

Dewangan, Gulab C.; Pal, Main; Pawar, Pramod +1 more

The broadband X-ray emission from type 1 active galactic nuclei, dominated by a power-law continuum, is thought to arise from repeated inverse Compton scattering of seed optical/UV photons by energetic electrons in a hot corona. The seed optical/UV photons are assumed to arise from an accretion disk, but direct observational evidence has remained …

2019 The Astrophysical Journal
XMM-Newton 12
Measuring the expansion and age of the nova shell IPHASX J210204.7 + 471015
DOI: 10.1093/mnras/sty3364 Bibcode: 2019MNRAS.483.3773S

Guerrero, M. A.; Toalá, J. A.; Santamaría, E. +4 more

The parallax expansion and kinematics of a nova shell can be used to assess its age and distance, and to investigate the interaction of the ejecta with the circumstellar medium. These are key to understand the expansion and dispersal of the nova ejecta in the Galaxy. Multi-epoch images and high-dispersion spectroscopic observations of the recently…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 12
First Evidence of Enhanced Recombination in Astrophysical Environments and the Implications for Plasma Diagnostics
DOI: 10.3847/2041-8213/ab5954 Bibcode: 2019ApJ...887L...9N

Dupree, A. K.; Raymond, J.; García-Rojas, J. +6 more

We report the first unambiguous observational evidence of Rydberg Enhanced Recombination (RER), a potentially important recombination mechanism that has hitherto been unexplored in low-temperature photoionized plasmas. RER shares similarities with dielectronic recombination, with the difference that the electron is captured into a highly excited s…

2019 The Astrophysical Journal
IUE 12
Migrating Scarps as a Significant Driver for Cometary Surface Evolution
DOI: 10.1029/2019GL083982 Bibcode: 2019GeoRL..4612794B

Soderblom, J. M.; Davidsson, B.; Oklay, N. +10 more

Rosetta observations of 67P/Churyumov-Gerasimenko (67P) reveal that most changes occur in the fallback-generated smooth terrains, vast deposits of granular material blanketing the comet's northern hemisphere. These changes express themselves both morphologically and spectrally across the nucleus, yet we lack a model that describes their formation …

2019 Geophysical Research Letters
Rosetta 12