Search Publications

The nuclear environment of the NLS1 Mrk 335: Obscuration of the X-ray line emission by a variable outflow
DOI: 10.1093/mnras/stz2566 Bibcode: 2019MNRAS.490..683P

Harrison, F. A.; Schartel, N.; Santos-Lleó, M. +12 more

We present XMM-Newton, NuSTAR, Swift, and Hubble Space Telescope observations of the Narrow-line Seyfert 1 galaxy Mrk 335 in a protracted low state in 2018 and 2019. The X-ray flux is at the lowest level so far observed, and the extremely low continuum flux reveals a host of soft X-ray emission lines from photoionized gas. The simultaneous UV flux…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 41
The structure of the Mg II broad line emitting region in Type 1 AGNs
DOI: 10.1093/mnras/stz157 Bibcode: 2019MNRAS.484.3180P

Popović, Luka Č.; Kovačević-Dojčinović, Jelena; Marčeta-Mandić, Sladjana

We investigate the structure of the Mg II broad line emission region in a sample of 284 Type 1 active galactic nuclei (AGNs), through comparing the kinematical parameters of the broad Mg II and broad Hβ lines. We found that the Mg II emitting region has more complex kinematics than the Hβ one. It seems that the Mg II broad line originates from two…

2019 Monthly Notices of the Royal Astronomical Society
eHST 41
Benchmark ages for the Gaia benchmark stars
DOI: 10.1093/mnras/sty2732 Bibcode: 2019MNRAS.482..895S

Feltzing, Sofia; Lindegren, Lennart; Sahlholdt, Christian L. +1 more

In the era of large-scale surveys of stars in the Milky Way, stellar ages are crucial for studying the evolution of the Galaxy. But determining ages of field stars is notoriously difficult; therefore, we attempt to determine benchmark ages for the extensively studied Gaia benchmark stars which can be used for validation purposes. By searching the …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 40
A statistically significant lack of debris discs in medium separation binary systems
DOI: 10.1093/mnras/stz1927 Bibcode: 2019MNRAS.488.3588Y

Wyatt, Mark C.; Kennedy, Grant M.; Su, Kate Y. L. +1 more

We compile a sample of 341 binary and multiple star systems with the aim of searching for and characterizing Kuiper belt-like debris discs. The sample is assembled by combining several smaller samples studied in previously published work with targets from two unpublished Herschel surveys. We find that 38 systems show excess emission at 70 or 100 &…

2019 Monthly Notices of the Royal Astronomical Society
AKARI Gaia Herschel 40
Random Forest identification of the thin disc, thick disc, and halo Gaia-DR2 white dwarf population
DOI: 10.1093/mnras/stz814 Bibcode: 2019MNRAS.485.5573T

Solano, E.; Rebassa-Mansergas, A.; Torres, S. +3 more

Gaia-DR2 has provided an unprecedented number of white dwarf candidates of our Galaxy. In particular, it is estimated that Gaia-DR2 has observed nearly 400 000 of these objects and close to 18 000 up to 100 pc from the Sun. This large quantity of data requires a thorough analysis in order to uncover their main Galactic population properties, in pa…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 40
OCCASO - III. Iron peak and α elements of 18 open clusters. Comparison with chemical evolution models and field stars
DOI: 10.1093/mnras/stz2595 Bibcode: 2019MNRAS.490.1821C

Jordi, C.; Casamiquela, L.; Anders, F. +10 more

The study of open-cluster chemical abundances provides insights on stellar nucleosynthesis processes and on Galactic chemo-dynamical evolution. In this paper we present an extended abundance analysis of 10 species (Fe, Ni, Cr, V, Sc, Si, Ca, Ti, Mg, O) for red giant stars in 18 OCCASO clusters. This represents a homogeneous sample regarding the in…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 40
PAHs as tracers of the molecular gas in star-forming galaxies
DOI: 10.1093/mnras/sty2777 Bibcode: 2019MNRAS.482.1618C

Daddi, E.; Elbaz, D.; Gómez-Guijarro, C. +12 more

We combine new CO(1-0) line observations of 24 intermediate redshift galaxies (0.03 < z < 0.28) along with literature data of galaxies at 0 < z < 4 to explore scaling relations between the dust and gas content using polycyclic aromatic hydrocarbon (PAH) 6.2 µm (L6.2), CO (L^' }_CO), and infrared (LIR) lumino…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 40
A deep view of a fossil relic in the Galactic bulge: the Globular Cluster HP 1
DOI: 10.1093/mnras/stz003 Bibcode: 2019MNRAS.484.5530K

Bica, E.; Nardiello, D.; Barbuy, B. +7 more

HP 1 is an α-enhanced and moderately metal-poor bulge globular cluster with a blue horizontal branch. These combined characteristics make it a probable relic of the early star formation in the innermost Galactic regions. Here, we present a detailed analysis of a deep near-infrared (NIR) photometry of HP 1 obtained with the NIR GSAOI + GeMS camera …

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 39
Jets blowing bubbles in the young radio galaxy 4C 31.04
DOI: 10.1093/mnras/stz233 Bibcode: 2019MNRAS.484.3393Z

Groves, Brent; Mukherjee, Dipanjan; Wagner, Alexander Y. +5 more

We report the discovery of shocked molecular and ionized gas resulting from jet-driven feedback in the low-redshift (z = 0.0602) compact radio galaxy 4C 31.04 using near-IR imaging spectroscopy. 4C 31.04 is a ∼100 pc double-lobed Compact Steep Spectrum source believed to be a very young active galactic nucleus (AGN). It is hosted by a giant ellipt…

2019 Monthly Notices of the Royal Astronomical Society
eHST 39
Probing the final-stage progenitor evolution for Type IIP Supernova 2017eaw in NGC 6946
DOI: 10.1093/mnras/stz503 Bibcode: 2019MNRAS.485.1990R

Wang, Lifan; Wang, Xiaofeng; Zhang, Jujia +6 more

We presented a detailed analysis of progenitor properties of type IIP supernova 2017eaw in NGC 6946, based on the pre-explosion images and early-time observations obtained immediately after the explosion. An unusually red star, with MF814W = -6.9 mag and mF606W - mF814W = 2.9 ± 0.2 mag, can be identified at the SN …

2019 Monthly Notices of the Royal Astronomical Society
eHST 39