Search Publications

Star formation towards the southern cometary H II region IRAS 17256-3631
DOI: 10.1093/mnras/stv2832 Bibcode: 2016MNRAS.456.2425V

Chandrasekhar, T.; Vig, S.; Ghosh, S. K. +4 more

IRAS 17256-3631 is a southern Galactic massive star-forming region located at a distance of 2 kpc. In this paper, we present a multiwavelength investigation of the embedded cluster, the H II region, as well as the parent cloud. Radio images at 325, 610 and 1372 MHz were obtained using Giant Metrewave Radio Telescope, India while the near-infrared …

2016 Monthly Notices of the Royal Astronomical Society
Herschel 20
Spectroscopic study of the HgMn star HD 49606: the quest for binarity, abundance stratifications and magnetic field
DOI: 10.1093/mnras/stw923 Bibcode: 2016MNRAS.460.1999C

Giarrusso, M.; Leone, F.; Scalia, C. +4 more

In this paper, we present a multi-instrument analysis of the mercury-manganese star HD 49606. New spectroscopic observations have been obtained by us with Catania Astrophysical Observatory Spectropolarimeter (CAOS@OAC) and High Accuracy Radial Velocity Planet Searcher-North@Telescopio Nazionale Galileo (HARPS-N@TNG). Combining these observations w…

2016 Monthly Notices of the Royal Astronomical Society
IUE 20
H-ATLAS/GAMA: the nature and characteristics of optically red galaxies detected at submillimetre wavelengths
DOI: 10.1093/mnras/stv2767 Bibcode: 2016MNRAS.456.2221D

Cooray, A.; Hony, S.; De Zotti, G. +39 more

We combine Herschel/SPIRE submillimetre (submm) observations with existing multiwavelength data to investigate the characteristics of low-redshift, optically red galaxies detected in submm bands. We select a sample of galaxies in the redshift range 0.01 ≤ z ≤ 0.2, having >5σ detections in the SPIRE 250 µm submm waveband. Sources are then …

2016 Monthly Notices of the Royal Astronomical Society
Herschel 20
Population of post-nova supersoft X-ray sources
DOI: 10.1093/mnras/stv2359 Bibcode: 2016MNRAS.455..668S

Gilfanov, Marat; Bildsten, Lars; Soraisam, Monika D. +1 more

Novae undergo a supersoft X-ray phase of varying duration after the optical outburst. Such transient post-nova supersoft X-ray sources (SSSs) are the majority of the observed SSSs in M31. In this paper, we use the post-nova evolutionary models of Wolf et al. to compute the expected population of post-nova SSSs in M31. We predict that depending on …

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 20
The clustering amplitude of X-ray-selected AGN at z ∼ 0.8: evidence for a negative dependence on accretion luminosity
DOI: 10.1093/mnras/stw281 Bibcode: 2016MNRAS.457.4195M

Georgakakis, A.; Salvato, M.; Liu, Z. +5 more

The northern tile of the wide-area and shallow XMM-XXL X-ray survey field is used to estimate the average dark matter halo mass of relatively luminous X-ray-selected active galactic nucleus (AGN) [log {L}_X (2-10 keV)= 43.6^{+0.4}_{-0.4} erg s^{-1}] in the redshift interval z = 0.5-1.2. Spectroscopic follow-up observations of X-ray sources in the …

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 20
[Fe II] jets from intermediate-mass protostars in Carina
DOI: 10.1093/mnras/stw2296 Bibcode: 2016MNRAS.463.4344R

Smith, Nathan; Bally, John; Reiter, Megan

We present new HST/WFC3-IR narrow-band [Fe II] images of protostellar jets in the Carina Nebula. Combined with five previously published sources, we have a sample of 18 jets and two Herbig-Haro (HH) objects. All of the jets we targeted with Wide-Field Camera 3 (WFC3) show bright infrared [Fe II] emission, and a few Hα candidate jets are confirmed …

2016 Monthly Notices of the Royal Astronomical Society
eHST 20
High-resolution mapping of dust via extinction in the M31 bulge
DOI: 10.1093/mnras/stw778 Bibcode: 2016MNRAS.459.2262D

Lauer, Tod R.; Wang, Q. D.; Dalcanton, Julianne J. +5 more

We map the dust distribution in the central 180 arcsec (∼680 pc) region of the M31 bulge, based on HST WFC3 and ACS observations in ten bands from near-ultraviolet (2700 Å) to near-infrared (1.5 µm). This large wavelength coverage gives us great leverage to detect not only dense dusty clumps, but also diffuse dusty molecular gas. We fit a pi…

2016 Monthly Notices of the Royal Astronomical Society
Herschel eHST 20
The structure and evolution of a forming galaxy cluster at z = 1.62
DOI: 10.1093/mnras/stw602 Bibcode: 2016MNRAS.459..387H

Hartley, W. G.; Conselice, C. J.; Almaini, O. +4 more

We present a comprehensive picture of the Cl 0218.3-0510 protocluster at z = 1.623 across 10 comoving Mpc. Using filters that tightly bracket the Balmer and 4000 Å breaks of the protocluster galaxies we obtain precise photometric redshifts resulting in a protocluster galaxy sample that is 89 ± 5 per cent complete and has a contamination of only 12…

2016 Monthly Notices of the Royal Astronomical Society
eHST 20
The PEP survey: evidence for intense star-forming activity in the majority of radio-selected AGN at z ≳ 1
DOI: 10.1093/mnras/stv2645 Bibcode: 2016MNRAS.456..431M

Berta, S.; Lutz, D.; Popesso, P. +4 more

In order to investigate the far-infrared (FIR) properties of radio-active active galactic nuclei (AGN), we have considered three different fields where both radio and FIR observations are the deepest to date: GOODS-South, GOODS-North and the Lockman Hole. Out of a total of 92 radio-selected AGN, ∼64 per cent are found to have a counterpart in Hers…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 20
Radio variability in the Phoenix Deep Survey at 1.4 GHz
DOI: 10.1093/mnras/stw1486 Bibcode: 2016MNRAS.461.3314H

Gaensler, B. M.; Hancock, P. J.; Bell, M. E. +2 more

We use archival data from the Phoenix Deep Survey to investigate the variable radio source population above 1 mJy beam-1 at 1.4 GHz. Given the similarity of this survey to other such surveys we take the opportunity to investigate the conflicting results which have appeared in the literature. Two previous surveys for variability conducte…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 19