Search Publications

A NuSTAR and XMM-Newton Study of the Two Most Actively Star-forming Green Pea Galaxies (SDSS J0749+3337 and SDSS J0822+2241)
DOI: 10.3847/1538-4357/ab2bf6 Bibcode: 2019ApJ...881...48K

Imanishi, Masatoshi; Tanimoto, Atsushi; Ueda, Yoshihiro +4 more

We explore X-ray evidence for the presence of active galactic nuclei (AGNs) in the two most actively star-forming Green Pea galaxies (GPs), SDSS J0749+3337 and SDSS J0822+2241, which have star formation rates (SFRs) of 123 M yr-1 and 78 M yr-1, respectively. The GPs have red mid-infrared (MIR) spectr…

2019 The Astrophysical Journal
XMM-Newton 7
Signature of Stochastic Acceleration and Cooling Processes in an Outburst Phase of the TeV Blazar ON 231
DOI: 10.3847/1538-4357/ab2765 Bibcode: 2019ApJ...880...19K

Gupta, Alok C.; Wiita, Paul J.; Kalita, Nibedita +1 more

We present a detailed spectral and temporal study of the intermediate-type blazar ON 231 during the TeV outburst phase in 2008 June with observations performed by Swift and XMM-Newton. The X-ray flux of the source, which was significantly dominated by the soft photons (below 3-4 keV), varies between 27% and 38% on day timescales, while mild variat…

2019 The Astrophysical Journal
XMM-Newton 7
Optical spectroscopic classification of 35 hard X-ray sources from the Swift-BAT 70-month catalogue
DOI: 10.1007/s10509-019-3642-9 Bibcode: 2019Ap&SS.364..153M

Palazzi, E.; Minniti, D.; Masetti, N. +15 more

The nature of a substantial percentage (about one fifth) of hard X-ray sources discovered with the BAT instrument onboard the Neil Gehrels Swift Observatory (hereafter Swift) is unknown because of the lack of an identified longer-wavelength counterpart. Without such follow-up, an X-ray catalogue is of limited astrophysical value: we therefore emba…

2019 Astrophysics and Space Science
XMM-Newton 7
Gas phase SiO in the circumstellar environment of the recurrent nova T Coronae Borealis
DOI: 10.1093/mnras/stz1071 Bibcode: 2019MNRAS.486.3498E

Munari, U.; Gehrz, R. D.; Shahbandeh, M. +9 more

We report the discovery of the diatomic molecule SiO in the gas phase in the environment of the recurrent nova T Coronae Borealis. While some of the SiO is photospheric, a substantial portion must arise in the wind from the red giant component of T CrB. A simple fit to the SiO feature, assuming local thermodynamic equilibrium, suggests a SiO colum…

2019 Monthly Notices of the Royal Astronomical Society
AKARI 7
Accurate stellar parameters and distance to two evolved eclipsing binary systems, OGLE-BLG-ECL-123903 and OGLE-BLG-ECL-296596, towards the Galactic bulge
DOI: 10.1051/0004-6361/201834298 Bibcode: 2019A&A...621A..93S

Soszyński, I.; Smolec, R.; Thompson, I. B. +15 more


Aims: Our aim is to obtain high-accuracy measurements of the physical and orbital parameters of two evolved eclipsing binary systems, and to use these measurements to study their evolutionary status. We also aim to derive the distances to the systems by using a surface brightness-colour relation and compare these distances with the measuremen…

2019 Astronomy and Astrophysics
Gaia 7
Star-forming regions at the periphery of the supershell surrounding the Cyg OB1 association - II. ISM kinematics and YSOs in the star cluster vdB 130 region
DOI: 10.1093/mnras/stz986 Bibcode: 2019MNRAS.486.2449S

Wiebe, D. S.; Moiseev, A. V.; Lozinskaya, T. A. +4 more

We present an observational study of small-scale feedback processes operating in the star-forming region located in the wall of the expanding supershell around the Cyg OB1 association. The interstellar gas and dust content and pre-stellar populations in the vicinity of the open star cluster vdB 130 are analysed based on new optical and IR observat…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 7
Clues on Arp 142: The spiral-elliptical merger
DOI: 10.1093/mnras/stz1744 Bibcode: 2019MNRAS.488..830M

Mendes de Oliveira, Claudia; Firpo, Verónica; Torres-Flores, Sergio +3 more

Nearby merging pairs are unique laboratories in which one can study the gravitational effects on the individual interacting components. In this manuscript, we report the characterization of selected H II regions along the peculiar galaxy NGC 2936, member of the galaxy pair Arp 142, an E+S interaction, known as `The Penguin'. Using Gemini South spe…

2019 Monthly Notices of the Royal Astronomical Society
eHST 7
Long-standing Small-scale Reconnection Processes at Saturn Revealed by Cassini
DOI: 10.3847/2041-8213/ab4429 Bibcode: 2019ApJ...884L..14G

Coates, A. J.; Krupp, N.; Dougherty, M. K. +12 more

The internal mass source from the icy moon Enceladus in Saturn’s rapidly rotating magnetosphere drives electromagnetic dynamics in multiple spatial and temporal scales. The distribution and circulation of the internal plasma and associated energy are thus crucial in understanding Saturn’s magnetospheric environment. Magnetic reconnection is one of…

2019 The Astrophysical Journal
Cassini 7
Comet C/2018 V1 (Machholz-Fujikawa-Iwamoto): dislodged from the Oort Cloud or coming from interstellar space?
DOI: 10.1093/mnras/stz2229 Bibcode: 2019MNRAS.489..951D

de la Fuente Marcos, R.; de la Fuente Marcos, C.

The chance discovery of the first interstellar minor body, 1I/2017 U1 (`Oumuamua), indicates that we may have been visited by such objects in the past and that these events may repeat in the future. Unfortunately, minor bodies following nearly parabolic or hyperbolic paths tend to receive little attention: over 3/4 of those known have data-arcs sh…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 7
Testing the deltaic origin of fan deposits at Bradbury Crater, Mars
DOI: 10.1016/j.icarus.2018.09.024 Bibcode: 2019Icar..319..363B

Mustard, John F.; Goudge, Timothy A.; Milliken, Ralph E. +1 more

The stratigraphic architectures of three fan-shaped deposits at Bradbury crater, Mars were investigated to test the hypothesis that the deposits were formed in standing bodies of water. Quantitative stratigraphic methods were applied to the northernmost deposit, which displays meter-thick layering. Planes fit to exposed strata display a constant d…

2019 Icarus
MEx 7