Search Publications

Supernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray Signatures
DOI: 10.1007/s11214-014-0062-6 Bibcode: 2015SSRv..188..187S

Slane, Patrick; Castro, Daniel; Ellison, Donald C. +2 more

The giant molecular clouds (MCs) found in the Milky Way and similar galaxies play a crucial role in the evolution of these systems. The supernova explosions that mark the death of massive stars in these regions often lead to interactions between the supernova remnants (SNRs) and the clouds. These interactions have a profound effect on our understa…

2015 Space Science Reviews
ISO 69
Discovery of H I gas in a young radio galaxy at z = 0.44 using the Australian Square Kilometre Array Pathfinder
DOI: 10.1093/mnras/stv1532 Bibcode: 2015MNRAS.453.1249A

Forsyth, R.; Sault, R. J.; Heywood, I. +100 more

We report the discovery of a new 21-cm H I absorption system using commissioning data from the Boolardy Engineering Test Array of the Australian Square Kilometre Array Pathfinder (ASKAP). Using the 711.5-1015.5 MHz band of ASKAP we were able to conduct a blind search for the 21-cm line in a continuous redshift range between z = 0.4 and 1.0, which …

2015 Monthly Notices of the Royal Astronomical Society
Planck XMM-Newton 69
Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales
DOI: 10.1088/0004-637X/811/2/111 Bibcode: 2015ApJ...811..111M

McNamara, Brian R.; Miller, Eric D.; Fabian, Andrew C. +17 more

We present new ultraviolet, optical, and X-ray data on the Phoenix galaxy cluster (SPT-CLJ2344-4243). Deep optical imaging reveals previously undetected filaments of star formation, extending to radii of ∼50-100 kpc in multiple directions. Combined UV-optical spectroscopy of the central galaxy reveals a massive (2 × 109 M), …

2015 The Astrophysical Journal
eHST 69
The link between accretion mode and environment in radio-loud active galaxies
DOI: 10.1093/mnras/stv1807 Bibcode: 2015MNRAS.453.2682I

Hardcastle, M. J.; Croston, J. H.; Kraft, R. P. +3 more

The interactions between radio-loud AGN and their environments play an important rôle in galaxy and cluster evolution. Recent work has demonstrated fundamental differences between high- and low-excitation radio galaxies (HERGs and LERGs), and shown that they may have different relationships with their environments. In the Chandra Large Project ERA…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 69
Surface morphology of fans in the high-Arctic periglacial environment of Svalbard: Controls and processes
DOI: 10.1016/j.earscirev.2015.04.004 Bibcode: 2015ESRv..146..163D

Hauber, Ernst; Kleinhans, Maarten G.; de Haas, Tjalling +2 more

Fan-shaped landforms occur in all climatic regions on Earth. They have been extensively studied in many of these regions, but there are few studies on fans in periglacial, Arctic and Antarctic regions. Fans in such regions are exposed to many site-specific environmental conditions in addition to their geological and topographic setting: there can …

2015 Earth Science Reviews
MEx 69
X-Ray High-resolution Spectroscopy Reveals Feedback in a Seyfert Galaxy from an Ultra-fast Wind with Complex Ionization and Velocity Structure
DOI: 10.1088/2041-8205/813/2/L39 Bibcode: 2015ApJ...813L..39L

Costantini, E.; Guainazzi, M.; Giroletti, M. +5 more

Winds outflowing from active galactic nuclei (AGNs) may carry significant amounts of mass and energy out to their host galaxies. In this paper we report the detection of a sub-relativistic outflow observed in the narrow line Seyfert 1 galaxy IRAS 17020+4544 as a series of absorption lines corresponding to at least five absorption components with a…

2015 The Astrophysical Journal
XMM-Newton 69
Star formation properties of sub-mJy radio sources
DOI: 10.1093/mnras/stv1675 Bibcode: 2015MNRAS.453.1079B

Berta, S.; Lutz, D.; Andreani, P. +8 more

We investigate the star formation properties of ∼800 sources detected in one of the deepest radio surveys at 1.4 GHz. Our sample spans a wide redshift range (∼0.1-4) and about four orders of magnitude in star formation rate (SFR). It includes both star-forming galaxies (SFGs) and active galactic nuclei (AGNs), further divided into radio-quiet (RQ)…

2015 Monthly Notices of the Royal Astronomical Society
Herschel 69
On the Temporal Evolution of Spicules Observed with IRIS, SDO, and Hinode
DOI: 10.1088/0004-637X/806/2/170 Bibcode: 2015ApJ...806..170S

De Pontieu, B.; Rouppe van der Voort, L.; Pereira, T. M. D. +1 more

Spicules are ubiquitous, fast moving jets observed off-limb in chromospheric spectral lines. Combining the recently launched Interface Region Imaging Spectrograph with the Solar Dynamics Observatory and Hinode, we have a unique opportunity to study spicules simultaneously in multiple passbands and from a seeing free environment. This makes it poss…

2015 The Astrophysical Journal
Hinode IRIS 69
Type IIb Supernova 2013df Entering into an Interaction Phase: A Link between the Progenitor and the Mass Loss
DOI: 10.1088/0004-637X/807/1/35 Bibcode: 2015ApJ...807...35M

Folatelli, G.; Tanaka, M.; Phillips, M. M. +23 more

We report the late-time evolution of Type IIb supernova (SN IIb) 2013df. SN 2013df showed a dramatic change in its spectral features at ∼1 yr after the explosion. Early on it showed typical characteristics shared by SNe IIb/Ib/Ic dominated by metal emission lines, while later on it was dominated by broad and flat-topped Hα and He i emissions. The …

2015 The Astrophysical Journal
eHST 69
Hubble Tarantula Treasury Project. II. The Star-formation History of the Starburst Region NGC 2070 in 30 Doradus
DOI: 10.1088/0004-637X/811/2/76 Bibcode: 2015ApJ...811...76C

Anderson, J.; Zaritsky, D.; Lennon, D. J. +10 more

We present a study of the recent star formation (SF) of 30 Doradus in the Large Magellanic Cloud (LMC) using the panchromatic imaging survey Hubble Tarantula Treasury Project. In this paper we focus on the stars within 20 pc of the center of 30 Doradus, the starburst region NGC 2070. We recovered the SF history by comparing deep optical and near-i…

2015 The Astrophysical Journal
eHST 69