Search Publications

Emission-line stars in M31 from the SPLASH and PHAT surveys
DOI: 10.1093/mnras/stw2984 Bibcode: 2017MNRAS.465.4180P

Williams, Benjamin F.; Seth, Anil C.; Dalcanton, Julianne J. +7 more

We present a sample of 224 stars that emit Hα (Hα stars) in the Andromeda galaxy (M31). The stars were selected from ∼5000 spectra, collected as part of the Spectroscopic and Photometric Landscape of Andromeda's Stellar Halo survey using Keck II/DEIMOS. We used six-filter Hubble Space Telescope photometry from the Panchromatic Hubble Andromeda Tre…

2017 Monthly Notices of the Royal Astronomical Society
eHST 6
Multiwavelength observations of the Be/X-ray binary IGR J01217-7257 (=SXP 2.16) during outburst
DOI: 10.1093/mnras/stw3169 Bibcode: 2017MNRAS.466.1149B

Udalski, A.; Coe, M. J.; Bird, A. J. +6 more

We present simultaneous, multiwavelength observations of the Small Magellanic Cloud Be/XRB IGR J01217-7257 (=SXP 2.16) during outbursts in 2014, 2015 and 2016. We also present the results of the RXTE observations of the Small Magellanic Cloud during which the source was initially discovered with a periodicity of 2.1652 ± 0.0001 s that we associate…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 6
De-noising the galaxies in the Hubble XDF with EMPCA
DOI: 10.1093/mnras/stx1380 Bibcode: 2017MNRAS.471..750M

Maturi, Matteo

We present a method to model optical images of galaxies using expectation maximization principal components analysis. The method returns de-noised images, it relies on the data alone and does not assume any pre-established model or fitting formula. It preserves the statistical properties of the sample, minimizing possible biases. The precision of …

2017 Monthly Notices of the Royal Astronomical Society
eHST 6
Hard X-ray spectral investigations of gamma-ray bursts 120521C and 130606A at high-redshift z ∼ 6
DOI: 10.1093/mnras/stw3130 Bibcode: 2017MNRAS.466.4558Y

Tashiro, M. S.; Urata, Y.; Yasuda, T. +1 more

This study presents a temporal and spectral analysis of the prompt emission of two high-redshift gamma-ray bursts (GRBs), 120521C at z ∼ 6 and 130606A at z ∼ 5.91, using data obtained from the Swift-XRT/BAT and the Suzaku-WAM simultaneously. Based on follow-up XRT observations, the longest durations of the prompt emissions were approximately 80 s …

2017 Monthly Notices of the Royal Astronomical Society
Suzaku 6
A Herschel resolved debris disc around HD 105211
DOI: 10.1093/mnras/stx753 Bibcode: 2017MNRAS.468.4725H

Marshall, J. P.; Horner, J.; Marsden, S. C. +1 more

Debris discs are the dusty aftermath of planet formation processes around main-sequence stars. Analysis of these discs is often hampered by the absence of any meaningful constraint on the location and spatial extent of the disc around its host star. Multi-wavelength, resolved imaging ameliorates the degeneracies inherent in the modelling process, …

2017 Monthly Notices of the Royal Astronomical Society
Herschel 6
Probing the cold and warm molecular gas in the Whirlpool Galaxy: Herschel SPIRE-FTS observations of the central region of M51 (NGC 5194)
DOI: 10.1093/mnras/stx1554 Bibcode: 2017MNRAS.470.4989S

Cooray, A.; De Looze, I.; Wu, R. +12 more

We present Herschel Spectral and Photometric Imaging Receiver (SPIRE)-Fourier Transform Spectrometer (FTS) intermediate-sampled mapping observations of the central ∼8 kpc (∼150 arcsec) of M51, with a spatial resolution of 40 arcsec. We detect four 12CO transitions (J = 4-3 to J = 7-6) and the [C I] 3P2-3

2017 Monthly Notices of the Royal Astronomical Society
Herschel 6
Three-dimensional Aquila Rift: magnetized H I arch anchored by molecular complex
DOI: 10.1093/mnras/stw2310 Bibcode: 2017MNRAS.464..783S

Nakanishi, Hiroyuki; Sofue, Yoshiaki

Three-dimensional structure of the Aquila Rift of magnetized neutral gas is investigated by analysing H I and CO line data. The projected distance on the Galactic plane of the H I arch of the Aquila Rift is r ∼ 250 pc from the Sun. The H I arch emerges at l ∼ 30°, reaches to altitudes as high as ∼500 pc above the plane at l ∼ 350°, and…

2017 Monthly Notices of the Royal Astronomical Society
Planck 6
An infrared photometric and spectroscopic study of post-AGB stars
DOI: 10.1093/mnras/stx1237 Bibcode: 2017MNRAS.470.1593R

Janardhan, P.; Pandey, R.; Anandarao, B. G. +1 more

We present here Spitzer mid-infrared (IR) spectra and modelling of the spectral energy distribution (SED) of a selection of post-asymptotic giant branch (PAGB) stars. The mid-IR spectra of the majority of these sources showed spectral features such as polycyclic aromatic hydrocarbons (PAHs) and silicates in emission. Our results from SED modelling…

2017 Monthly Notices of the Royal Astronomical Society
AKARI ISO 6
High-resolution spectroscopy and abundance analysis of δ Scuti stars near the γ Doradus instability strip
DOI: 10.1093/mnras/stx1498 Bibcode: 2017MNRAS.470.4408K

Kambe, E.; Niemczura, E.; Molenda-Żakowicz, J. +5 more

δ Scuti stars are remarkable objects for asteroseismology. In spite of decades of investigations, there are still important questions about these pulsating stars to be answered, such as their positions in log Teff-log g diagram, or the dependence of the pulsation modes on atmospheric parameters and rotation. Therefore, we performed a de…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 6
Investigating the nature of the INTEGRAL gamma-ray bursts and sub-threshold triggers with Swift follow-up
DOI: 10.1093/mnras/stx1163 Bibcode: 2017MNRAS.470..314H

Götz, D.; Mereghetti, S.; Gehrels, N. +9 more

We explore the potential of the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) to improve our understanding of the low-fluence regime for explosive transients, such as Gamma-ray Bursts (GRBs). We probe the nature of the so-called 'WEAK' INTEGRAL triggers, when the gamma-ray instruments record intensity spikes that are below the usual S…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 6