Search Publications

Catching jetted tidal disruption events early in millimetre
DOI: 10.1093/mnras/stw1543 Bibcode: 2016MNRAS.461.3375Y

Yuan, Qiang; Wang, Q. Daniel; Zhang, Bing +2 more

Relativistic jets can form from at least some tidal disruption events (TDEs) of (sub-)stellar objects around supermassive black holes. We detect the millimetre (MM) emission of IGR J12580+0134 - the nearest TDE known in the galaxy NGC 4845 at the distance of only 17 Mpc, based on Planck all-sky survey data. The data show significant flux jumps aft…

2016 Monthly Notices of the Royal Astronomical Society
Planck 22
Distinguishing disks from mergers: Tracing the kinematic asymmetries in local (U)LIRGs using kinemetry-based criteria
DOI: 10.1051/0004-6361/201526974 Bibcode: 2016A&A...591A..85B

Arribas, Santiago; Colina, Luis; Bellocchi, Enrica

Context. The kinematic characterization of different galaxy populations is a key observational input for distinguishing between different galaxy evolutionary scenarios because it helps to determine the number ratio of rotating disks to mergers at different cosmic epochs. Local (ultra) luminous infrared galaxies ((U)LIRGs) cover similar range of st…

2016 Astronomy and Astrophysics
eHST 22
To v and beyond! The He I absorption variability across the 2014.6 periastron passage of η Carinae
DOI: 10.1093/mnras/stw1415 Bibcode: 2016MNRAS.461.2540R

Hamaguchi, Kenji; Corcoran, Michael F.; Russell, Christopher M. P. +11 more

We have monitored the massive binary star η Carinae with the CTIO/Small and Moderate Aperture Research Telescope System 1.5 m telescope and CHIRON spectrograph from the previous apastron passage of the system through the recent 2014.6 periastron passage. Our monitoring has resulted in a large, homogeneous data set with an unprecedented time-sampli…

2016 Monthly Notices of the Royal Astronomical Society
eHST 22
Imprint of inhomogeneous and anisotropic primordial power spectrum on CMB polarization
DOI: 10.1093/mnras/stw1039 Bibcode: 2016MNRAS.460.1577K

Ghosh, Shamik; Kothari, Rahul; Jain, Pankaj +2 more

We consider an inhomogeneous model and independently an anisotropic model of primordial power spectrum in order to describe the observed hemispherical anisotropy in cosmic microwave background radiation (CMBR). This anisotropy can be parametrized in terms of the dipole modulation model of the temperature field. Both the models lead to correlations…

2016 Monthly Notices of the Royal Astronomical Society
Planck 22
Determining Type Ia Supernova Host Galaxy Extinction Probabilities and a Statistical Approach to Estimating the Absorption-to-reddening Ratio RV
DOI: 10.3847/0004-637X/819/2/152 Bibcode: 2016ApJ...819..152C

Marleau, Francine; Deustua, Susana; Cikota, Aleksandar

We investigate limits on the extinction values of Type Ia supernovae (SNe Ia) to statistically determine the most probable color excess, E(B - V), with galactocentric distance, and use these statistics to determine the absorption-to-reddening ratio, RV, for dust in the host galaxies. We determined pixel-based dust mass surface density m…

2016 The Astrophysical Journal
Herschel eHST 22
The Circum-Galactic Medium of MASsive Spirals. I. An Overview and a Case Study of NGC 5908
DOI: 10.3847/0004-637X/830/2/134 Bibcode: 2016ApJ...830..134L

Bregman, Joel N.; Anderson, Michael E.; Crain, Robert A. +2 more

The Circum-Galactic Medium of MASsive Spirals is a project studying the overall content, physical and chemical properties, and spatial distributions of the multi-phase circumgalactic medium around a small sample of the most massive ({M}* ≳ 2× {10}11 {M}, {v}{rot}\gt 300 {km} {{{s}}}-1) isola…

2016 The Astrophysical Journal
XMM-Newton 22
Evidence for a chemical enrichment coupling of globular clusters and field stars in the Fornax dSph
DOI: 10.1051/0004-6361/201526996 Bibcode: 2016A&A...585A..86H

Johnson, Christian I.; Mateo, Mario; Frank, Matthias J. +4 more

The globular cluster H4, located in the center of the Fornax dwarf spheroidal galaxy, is crucial for understanding the formation and chemical evolution of star clusters in low-mass galactic environments. H4 is peculiar because the cluster is significantly more metal-rich than the galaxy's other clusters, is located near the galaxy center, and may …

2016 Astronomy and Astrophysics
eHST 22
GeMS/GSAOI Photometric and Astrometric Performance in Dense Stellar Fields
DOI: 10.3847/1538-4357/833/1/111 Bibcode: 2016ApJ...833..111D

Dalessandro, E.; Saracino, S.; Marchetti, E. +7 more

Ground-based imagers at 8 m class telescopes assisted by multi-conjugate adaptive optics are primary facilities with which to obtain accurate photometry and proper motions in dense stellar fields. We observed the central region of the globular clusters Liller 1 and NGC 6624 with the Gemini Multi-conjugate Adaptive Optics System (GeMS) feeding the …

2016 The Astrophysical Journal
eHST 21
Time-dependent tomographic reconstruction of the solar corona
DOI: 10.1016/j.ascom.2016.09.001 Bibcode: 2016A&C....17..144V

Lamy, P.; Vibert, D.; Peillon, C. +2 more

Solar rotational tomography (SRT) applied to white-light coronal images observed at multiple aspect angles has been the preferred approach for determining the three-dimensional (3D) electron density structure of the solar corona. However, it is seriously hampered by the restrictive assumption that the corona is time-invariant which introduces sign…

2016 Astronomy and Computing
SOHO 21
Discovery of Ubiquitous Fast-Propagating Intensity Disturbances by the Chromospheric Lyman Alpha Spectropolarimeter (CLASP)
DOI: 10.3847/0004-637X/832/2/141 Bibcode: 2016ApJ...832..141K

Auchère, F.; Giono, G.; Kubo, M. +25 more

High-cadence observations by the slit-jaw (SJ) optics system of the sounding rocket experiment known as the Chromospheric Lyman Alpha Spectropolarimeter (CLASP) reveal ubiquitous intensity disturbances that recurrently propagate in either the chromosphere or the transition region or both at a speed much higher than the speed of sound. The CLASP/SJ…

2016 The Astrophysical Journal
IRIS 21