Search Publications

Kinematics of powerful jets from intermediate-mass protostars in the Carina nebula
DOI: 10.1093/mnras/stu1979 Bibcode: 2014MNRAS.445.3939R

Smith, Nathan; Reiter, Megan

We present measurements of proper motions and radial velocities of four powerful Herbig-Haro (HH) jets in the Carina nebula: HH 666, HH 901, HH 902, and HH 1066. Two epochs of Hubble Space Telescope imaging separated by a time baseline of ∼4.4 yr provide proper motions that allow us to measure the transverse velocities of the jets, while ground-ba…

2014 Monthly Notices of the Royal Astronomical Society
eHST 12
A panchromatic survey of post-starburst mergers: searching for feedback
DOI: 10.1093/mnras/stu141 Bibcode: 2014MNRAS.439.2837D

De Propris, Roberto; Melnick, Jorge

We consider the morphology, stellar populations, structure and AGN activity of 10 post-starburst (K+A) galaxies with Hubble Space Telescope (HST) observations, full spectral coverage in the optical, spectral energy distributions from 0.2 to 160 µm, X-ray and radio data. Our results show that the post-starburst galaxy (PSG) phenomenon is rela…

2014 Monthly Notices of the Royal Astronomical Society
eHST 12
On the presence of ultrafast outflows in the WAX sample of Seyfert galaxies.
DOI: 10.1093/mnrasl/slu091 Bibcode: 2014MNRAS.443L.104T

Cappi, M.; Tombesi, F.

The study of winds in active galactic nuclei (AGNs) is of utmost importance as they may provide the long sought-after link between the central black hole and the host galaxy, establishing the AGN feedback. Recently, Laha et al. reported the X-ray analysis of a sample of 26 Seyferts observed with XMM-Newton, which are part of the so-called warm abs…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 12
Discovery of SXP 265, a Be/X-ray binary pulsar in the Wing of the Small Magellanic Cloud
DOI: 10.1093/mnras/stu1680 Bibcode: 2014MNRAS.444.3571S

Haberl, F.; Greiner, J.; Udalski, A. +5 more

We identify a new candidate for a Be/X-ray binary in the XMM-Newton slew survey and archival Swift observations that is located in the transition region of the Wing of the Small Magellanic Cloud and the Magellanic Bridge. We investigated and classified this source with follow-up XMM-Newton and optical observations. We model the X-ray spectra and s…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 12
Constraints to the magnetospheric properties of T Tauri stars - I. The C II], Fe II] and Si II] ultraviolet features
DOI: 10.1093/mnras/stu1045 Bibcode: 2014MNRAS.442.2951L

López-Martínez, Fatima; Gómez de Castro, Ana Inés

The C II] feature at ∼2325 Å is very prominent in the spectra of T Tauri stars (TTSs). This feature is a quintuplet of semiforbidden transitions excited at electron temperatures around 10 000 K that, together with the nearby Si II] and Fe II] features, provides a reliable optically thin tracer for accurate measurement of the plasma properties in t…

2014 Monthly Notices of the Royal Astronomical Society
eHST 12
The role of major mergers in the size growth of intermediate-mass spheroids
DOI: 10.1093/mnras/stu1220 Bibcode: 2014MNRAS.443.1861K

Ryan, R. E.; O'Connell, R. W.; Koekemoer, A. M. +11 more

We study of the role of `major' mergers (mass ratios >1: 4) in driving size growth in high-redshift (1 < z < 2) spheroidal galaxies (SGs) with stellar masses between 109.5 and 1010.7 M. This is a largely unexplored mass range at this epoch, containing the progenitors of more massive SGs on which the bulk …

2014 Monthly Notices of the Royal Astronomical Society
eHST 12
Emission mechanism of GeV-quiet soft gamma-ray pulsars: a case for peculiar geometry?
DOI: 10.1093/mnras/stu1765 Bibcode: 2014MNRAS.445..604W

Leung, Gene C. K.; Cheng, K. S.; Takata, J. +2 more

There is a growing new class of young spin-down powered pulsars called GeV-quiet soft gamma-ray pulsar; (1) spectral turnover appears around 10 MeV, (2) the X-ray spectra of below 20 keV can be described by power law with a photon index of around 1.2 and (3) the light curve in X-ray/soft gamma-ray bands shows single broad pulse. Their emission pro…

2014 Monthly Notices of the Royal Astronomical Society
INTEGRAL 12
Non-Gaussianity of the cosmic infrared background anisotropies - II. Predictions of the bispectrum and constraints forecast
DOI: 10.1093/mnras/stt2372 Bibcode: 2014MNRAS.439..143P

Aghanim, N.; Lacasa, F.; Pénin, A.

Using a full analytical computation of the bispectrum based on the halo model together with the halo occupation number, we derive the bispectrum of the cosmic infrared background (CIB) anisotropies that trace the clustering of dusty-star-forming galaxies. We focus our analysis on wavelengths in the far-infrared and the sub-millimeter typical of th…

2014 Monthly Notices of the Royal Astronomical Society
Planck 12
Molecular gas properties of UV-bright star-forming galaxies at low redshift
DOI: 10.1093/mnras/stu852 Bibcode: 2014MNRAS.442.1429G

Basu-Zych, Antara; Overzier, Roderik A.; Martin, D. Christopher +2 more

Lyman break analogues (LBAs) are a population of star-forming galaxies at low redshift (z ∼ 0.2) selected in the ultraviolet (UV). These objects present higher star formation rates and lower dust extinction than other galaxies with similar masses and luminosities in the local universe. In this work, we present results from a survey with the Combin…

2014 Monthly Notices of the Royal Astronomical Society
eHST 12
The Herschel view of circumstellar discs: a multiwavelength study of Chamaeleon-I
DOI: 10.1093/mnras/stu908 Bibcode: 2014MNRAS.443.1587R

Ray, Tom; Scholz, Alexander; Rodgers-Lee, Donna +1 more

We present the results of a multiwavelength study of circumstellar discs around 44 young stellar objects in the 3 myr old nearby Chamaeleon-I star-forming region. In particular, we explore the far-infrared/submm regime using Herschel fluxes. We show that Herschel fluxes at 160-500 µm can be used to derive robust estimates of the disc mass. T…

2014 Monthly Notices of the Royal Astronomical Society
Herschel 11