Search Publications

A New Method for Wide-field Near-IR Imaging with the Hubble Space Telescope
DOI: 10.1088/1538-3873/129/971/015004 Bibcode: 2017PASP..129a5004M

van Dokkum, Pieter G.; Franx, Marijn; Muzzin, Adam +6 more

We present a new technique for wide and shallow observations using the near-infrared channel of Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST). Wide-field near-IR surveys with HST are generally inefficient, as guide star acquisitions make it impractical to observe more than one pointing per orbit. This limitation can be circumvente…

2017 Publications of the Astronomical Society of the Pacific
eHST 29
Pre-flare coronal dimmings
DOI: 10.1051/0004-6361/201629477 Bibcode: 2017A&A...598A...3Z

Ji, H. S.; Zhang, Q. M.; Su, Y. N.

Context. Coronal dimmings are regions of decreased extreme-ultravoilet (EUV) and/or X-ray (originally Skylab, then Yohkoh/SXT) intensities, which are often associated with flares and coronal mass ejections (CMEs). The large-scale impulsive dimmings have been thoroughly observed and investigated. The pre-flare dimmings before the flare impulsive ph…

2017 Astronomy and Astrophysics
SOHO 29
The 2015 outburst of the accretion-powered pulsar IGR J00291+5934: INTEGRAL and Swift observations
DOI: 10.1051/0004-6361/201629575 Bibcode: 2017A&A...599A..88D

Stella, L.; Ferrigno, C.; Bozzo, E. +5 more

The pulsar IGR J00291+5934 is the fastest-known accretion-powered X-ray pulsar, discovered during a transient outburst in 2004. In this paper, we report on INTEGRAL and Swift observations during the 2015 outburst, which lasts for 25 d. The source has not been observed in outburst since 2008, suggesting that the long-term accretion rate has decreas…

2017 Astronomy and Astrophysics
INTEGRAL 29
Dynamical histories of the IC 348 and NGC 1333 star-forming regions in Perseus
DOI: 10.1093/mnras/stx739 Bibcode: 2017MNRAS.468.4340P

Parker, Richard J.; Alves de Oliveira, Catarina

We present analyses of the spatial distributions of stars in the young (1-3 Myr) star-forming regions IC 348 and NGC 1333 in the Perseus giant molecular cloud. We quantify the spatial structure using the Q-parameter and find that both IC 348 and NGC 1333 are smooth and centrally concentrated with Q-parameters of 0.98 and 0.89, respectively. Neithe…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 29
Mapping young stellar populations toward Orion with Gaia DR1
DOI: 10.1051/0004-6361/201731309 Bibcode: 2017A&A...608A.148Z

Brown, A. G. A.; Manara, C. F.; de Zeeuw, P. T. +2 more

In this work we use the first data release of the Gaia mission to explore the three-dimensional arrangement and age ordering of the many stellar groups toward the Orion OB association, aiming at a new classification and characterization of the stellar population not embedded in the Orion A and B molecular clouds. We make use of the parallaxes and …

2017 Astronomy and Astrophysics
Gaia Planck 29
Comparing Automatic CME Detections in Multiple LASCO and SECCHI Catalogs
DOI: 10.3847/1538-4357/aa5b85 Bibcode: 2017ApJ...836..134H

Hess, Phillip; Colaninno, Robin C.

With the creation of numerous automatic detection algorithms, a number of different catalogs of coronal mass ejections (CMEs) spanning the entirety of the Solar and Heliospheric Observatory (SOHO) Large Angle Spectrometric Coronagraph (LASCO) mission have been created. Some of these catalogs have been further expanded for use on data from the Sola…

2017 The Astrophysical Journal
SOHO 29
New Insights in the Mid-infrared Bubble N49 Site: A Clue of Collision of Filamentary Molecular Clouds
DOI: 10.3847/1538-4357/aa9be2 Bibcode: 2017ApJ...851..140D

Dewangan, L. K.; Ojha, D. K.; Zinchenko, I.

We investigate the star formation processes operating in a mid-infrared bubble N49 site that harbors an O-type star in its interior, an ultracompact H II region, and a 6.7 GHz methanol maser at its edges. The 13CO line data reveal two velocity components (at velocity peaks ∼88 and ∼95 km s-1) in the direction of the bubble. A…

2017 The Astrophysical Journal
Herschel 29
Large decay of X-ray flux in 2XMM J123103.2+110648: evidence for a tidal disruption event
DOI: 10.1093/mnras/stx489 Bibcode: 2017MNRAS.468..783L

Ho, Luis C.; Lin, Dacheng; Godet, Olivier +3 more

The X-ray source 2XMM J123103.2+110648 was previously found to show pure thermal X-ray spectra and an ∼3.8 h periodicity in three XMM-Newton X-ray observations in 2003-2005, and the optical spectrum of the host galaxy suggested it as a type 2 active galactic nucleus candidate. We have obtained new X-ray observations of the source, with Swift and C…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 29
The Spectroscopy and H-band Imaging of Virgo Cluster Galaxies (SHIVir) Survey: Scaling Relations and the Stellar-to-total Mass Relation
DOI: 10.3847/1538-4357/aa74b1 Bibcode: 2017ApJ...843...74O

Taylor, James E.; Holtzman, Jon A.; Cappellari, Michele +10 more

We present parameter distributions and fundamental scaling relations for 190 Virgo cluster galaxies in the SHIVir survey. The distribution of galaxy velocities is bimodal about V circ ∼ 125 km s-1, hinting at the existence of dynamically unstable modes in the inner regions of galaxies. An analysis of the Tully-Fisher relation…

2017 The Astrophysical Journal
eHST 29
Dipolar modulation in the size of galaxies: the effect of Doppler magnification
DOI: 10.1093/mnras/stx2049 Bibcode: 2017MNRAS.472.3936B

Bacon, David; Bonvin, Camille; Andrianomena, Sambatra +4 more

Objects falling into an overdensity appear larger on its near side and smaller on its far side than other objects at the same redshift. This produces a dipolar pattern of magnification, primarily as a consequence of the Doppler effect. At low redshift, this Doppler magnification completely dominates the usual integrated gravitational lensing contr…

2017 Monthly Notices of the Royal Astronomical Society
Planck 29