Search Publications

Post-flare formation of the accretion stream and a dip in pulse profiles of LMC X-4
DOI: 10.1016/j.newast.2017.05.001 Bibcode: 2017NewA...56...94B

Paul, Biswajit; Beri, Aru

We report here a pulse profile evolution study of an accreting X-ray pulsar LMC X-4 during and after the large X-ray flares using data from the two observatories XMM-Newton and RXTE. During the flares, the pulse profiles were found to have a significant phase offset in the range of 0.2-0.5 compared to the pulse profiles immediately before or after…

2017 New Astronomy
XMM-Newton 12
Detection of Prominent Stellar Disks in the Progenitors of Present-day Massive Elliptical Galaxies
DOI: 10.3847/1538-4357/836/1/75 Bibcode: 2017ApJ...836...75D

Ho, Luis C.; Mobasher, Bahram; Canalizo, Gabriela +1 more

Massive galaxies at high redshifts (z > 2) show different characteristics from their local counterparts: they are compact and most likely have a disk. In this study, we trace the evolution of local massive galaxies by performing a detailed morphological analysis, namely, fitting single Sérsic profiles and performing bulge+disk decompositions. W…

2017 The Astrophysical Journal
eHST 12
CTIO, ROSAT HRI, and Chandra ACIS Observations of the Archetypical Mixed-morphology Supernova Remnant W28 (G6.4-0.1)
DOI: 10.3847/1538-4357/aa615c Bibcode: 2017ApJ...839...59P

Kargaltsev, Oleg; Rho, Jeonghee; Hare, Jeremy +6 more

We present a joint analysis of optical emission-line and X-ray observations of the archetypical Galactic mixed-morphology supernova remnant (MMSNR) W28 (G6.4-0.1). MMSNRs comprise a class of sources whose shell-like radio morphology contrasts with a filled center in X-rays; the origin of these contrasting morphologies remains uncertain. Our CTIO i…

2017 The Astrophysical Journal
XMM-Newton 12
The effect of unresolved contaminant stars on the cross-matching of photometric catalogues
DOI: 10.1093/mnras/stx629 Bibcode: 2017MNRAS.468.2517W

Wilson, Tom J.; Naylor, Tim

A fundamental process in astrophysics is the matching of two photometric catalogues. It is crucial that the correct objects be paired, and that their photometry does not suffer from any spurious additional flux. We compare the positions of sources in Wide-field Infrared Survey Explorer (WISE), INT Photometric H α Survey, Two Micron All Sky Survey …

2017 Monthly Notices of the Royal Astronomical Society
Gaia 12
Multi-spacecraft Observations of the Coronal and Interplanetary Evolution of a Solar Eruption Associated with Two Active Regions
DOI: 10.3847/1538-4357/aa6d54 Bibcode: 2017ApJ...840...76H

Wang, Rui; Yang, Zhongwei; Liu, Ying D. +3 more

We investigate the coronal and interplanetary evolution of a coronal mass ejection (CME) launched on 2010 September 4 from a source region linking two active regions (ARs), 11101 and 11103, using extreme ultraviolet imaging, magnetogram, white-light, and in situ observations from SDO, STEREO, SOHO, VEX, and Wind. A potential-field source-surface m…

2017 The Astrophysical Journal
SOHO VenusExpress 12
Simulated Galactic methanol maser distribution to constrain Milky Way parameters
DOI: 10.1051/0004-6361/201730681 Bibcode: 2017A&A...604A..72Q

Reid, M. J.; Quiroga-Nuñez, L. H.; van Langevelde, H. J. +1 more

Context. Using trigonometric parallaxes and proper motions of masers associated with massive young stars, the Bar and Spiral Structure Legacy (BeSSeL) survey has reported the most accurate values of the Galactic parameters so far. The determination of these parameters with high accuracy has a widespread impact on Galactic and extragalactic measure…

2017 Astronomy and Astrophysics
Gaia 12
The outflow of gas from the Centaurus A circumnuclear disk. Atomic spectral line maps from Herschel/PACS and APEX
DOI: 10.1051/0004-6361/201629396 Bibcode: 2017A&A...599A..53I

Stutzki, J.; Güsten, R.; Requena-Torres, M. A. +2 more

The physical state of the gas in the central 500 pc of NGC 5128 (the radio galaxy Centaurus A), was investigated using the fine-structure lines of carbon [CI], [CII]; oxygen [OI], [OIII], and nitrogen [NII], [NIII] as well as the 12CO(4-3) molecular line. The circumnuclear disk (CND) is traced by emission from dust and the neutral gas (…

2017 Astronomy and Astrophysics
Herschel 12
Statistical study of polar negative magnetic bays driven by interplanetary fast-mode shocks
DOI: 10.1002/2017JA024465 Bibcode: 2017JGRA..122.7463L

Liou, Kan; Sotirelis, Thomas; Gjerloev, Jesper

The question of whether an interplanetary (IP) fast-mode shock can trigger the substorm expansion is still not resolved. Some scientists believe that the substorm expansion can be triggered by a sudden compression of the magnetosphere if a substorm growth phase is in progress (e.g., the magnetosphere precondition hypothesis). Such a hypothesis has…

2017 Journal of Geophysical Research (Space Physics)
Cluster 12
Physical Properties of the Very Young PN Hen3-1357 (Stingray Nebula) Based on Multiwavelength Observations
DOI: 10.3847/1538-4357/aa64d0 Bibcode: 2017ApJ...838...71O

Hubrig, S.; Otsuka, Masaaki; Parthasarathy, M. +1 more

We carried out a detailed analysis of the interesting and important very young planetary nebula (PN) Hen3-1357 (Stingray Nebula) based on a unique data set of optical to far-IR spectra and photometric images. We calculated the abundances of nine elements using collisionally excited lines (CELs) and recombination lines (RLs). The RL C/O ratio indic…

2017 The Astrophysical Journal
eHST 12
A catalogue of white dwarf candidates in VST ATLAS
DOI: 10.1093/mnras/stx777 Bibcode: 2017MNRAS.469..621G

Hermes, J. J.; Raddi, Roberto; Gänsicke, Boris T. +6 more

The Sloan Digital Sky Survey (SDSS) has created a knowledge gap between the Northern and the Southern hemispheres, which is very marked for white dwarfs: Only ≃15 per cent of the known white dwarfs are south of the equator. Here, we make use of the VLT Survey Telescope (VST) ATLAS survey, one of the first surveys obtaining deep, optical, multiband…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 12