Search Publications

Fine structures at pore boundary
DOI: 10.1093/mnrasl/slw130 Bibcode: 2016MNRAS.462L..93B

Bharti, L.; Quintero Noda, C.; Joshi, C. +2 more

We present high resolution observations of fine structures at pore boundaries. The inner part of granules towards umbra show dark striations which evolve into a filamentary structure with dark core and `Y' shape at the head of the filaments. These filaments migrate into the umbra similar to penumbral filaments. These filaments show higher temperat…

2016 Monthly Notices of the Royal Astronomical Society
Hinode 3
Observations of the planetary nebula RWT 152 with OSIRIS/GTC
DOI: 10.1093/mnras/stw1916 Bibcode: 2016MNRAS.462.3945A

Solano, E.; Ulla, A.; Miranda, L. F. +2 more

RWT 152 is one of the few known planetary nebulae with an sdO central star. We present subarcsecond red tunable filter Hα imaging and intermediate-resolution, long-slit spectroscopy of RWT 152 obtained with OSIRIS/GTC (Optical System for Imaging and low-Intermediate-Resolution Integrated Spectroscopy/Gran Telescopio Canarias) with the goal of anal…

2016 Monthly Notices of the Royal Astronomical Society
IUE 2
Fundamental stellar parameters for selected T-Tauri stars in the Chamaeleon and Rho Ophiuchus star-forming regions
DOI: 10.1093/mnras/stw481 Bibcode: 2016MNRAS.459.1363J

James, D. J.; Bouvier, J.; Santos, N. C. +4 more

We present the results of an optical photometry and high-resolution spectroscopy campaign for a modest sample of X-ray selected stars in the Chamaeleon and Rho Ophiuchus star-forming regions. With R∼ 50 000 optical spectra, we establish kinematic membership of the parent association and confirm stellar youth for each star in our sample. With the a…

2016 Monthly Notices of the Royal Astronomical Society
AKARI 2
Searching for X-ray sources in nearby late-type galaxies with low-star formation rates
DOI: 10.1093/mnras/stv2888 Bibcode: 2016MNRAS.456.2966C

Kaaret, P.; Poutanen, J.; Kajava, J. J. E. +4 more

Late-type non-starburst galaxies have been shown to contain X-ray emitting objects, some being ultraluminous X-ray sources. We report on XMM-Newton observations of 11 nearby, late-type galaxies previously observed with the Hubble Space Telescope (HST) in order to find such objects. We found 18 X-ray sources in or near the optical extent of the gal…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 2
Erratum: Discovery of H I gas in a young radio galaxy at z = 0.44 using the Australian Square Kilometre Array Pathfinder
DOI: 10.1093/mnras/stv2908 Bibcode: 2016MNRAS.456.3030A

Forsyth, R.; Sault, R. J.; Heywood, I. +100 more

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 2
Discovery of two new fast X-ray transients with INTEGRAL: IGR J03346+4414 and IGR J20344+3913
DOI: 10.1093/mnras/stw2183 Bibcode: 2016MNRAS.463.2885S

Sidoli, L.; Bird, A. J.; Paizis, A. +1 more

We report on the discovery of two fast X-ray transients (FXTs) from analysis of archival INTEGRAL data. Both are characterized by a remarkable hard X-ray activity above 20 keV, in terms of duration (∼15 and 30 min, respectively), peak flux (∼10-9 erg cm-2 s-1) and dynamic range (∼2400 and 1360, respectively). Swift…

2016 Monthly Notices of the Royal Astronomical Society
INTEGRAL 1
Searching for Faraday rotation in cosmic microwave background polarization
DOI: 10.1093/mnras/stw1157 Bibcode: 2016MNRAS.460.3089R

Battaner, E.; Ruiz-Granados, B.; Florido, E.

We use the Wilkinson Microwave Anisotropy Probe (WMAP) 9th-year foreground reduced data at 33, 41 and 61 GHz to derive a Faraday rotation at map and at angular power spectrum levels taking into account their observational errors. A processing mask provided by WMAP is used to avoid contamination from the disc of our Galaxy and local spurs. We have …

2016 Monthly Notices of the Royal Astronomical Society
Planck 1
2D photochemical model for forbidden oxygen line emission for comet 1P/Halley
DOI: 10.1093/mnras/stw2150 Bibcode: 2016MNRAS.462S.116C

Gunell, H.; Rubin, M.; De Keyser, J. +8 more

We present here a 2D model of photochemistry for computing the production and loss mechanisms of the O(1S) and O(1D) states, which are responsible for the emission lines at 577.7, 630, and 636.4 nm, in case of the comet 1P/Halley. The presence of O2 within cometary atmospheres, measured by the in situ Rosetta and G…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 1
A new investigation of the possible X-ray counterparts of the magnetar candidate AX J1845-0258
DOI: 10.1093/mnras/stw1036 Bibcode: 2016MNRAS.460.1033P

Pintore, Fabio; Mereghetti, Sandro

AX J1845-0258 is a transient X-ray pulsar, with spin period of 6.97 s, discovered with the ASCA satellite in 1993. Its soft spectrum and the possible association with a supernova remnant suggest that AX J1845-0258 might be a magnetar, but this has not been confirmed yet. A possible counterpart one order of magnitude fainter, AX J184453-025640, has…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 1
ERRATUM: `The variable spin-down rate of the transient magnetar XTE J1810-197'
DOI: 10.1093/mnras/stw928 Bibcode: 2016MNRAS.459.3620P

Pintore, Fabio; Mereghetti, Sandro; Esposito, Paolo +7 more

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 1