Search Publications

Witnessing Gas Mixing in the Metal Distribution of the Hickson Compact Group HCG 31
DOI: 10.1088/2041-8205/798/1/L24 Bibcode: 2015ApJ...798L..24T

Mendes de Oliveira, C.; de Mello, D. F.; Amram, P. +3 more

We present for the first time direct evidence that in a merger of disk galaxies, the pre-existing central metallicities will mix as a result of gas being transported in the merger interface region along the line that joins the two coalescing nuclei. This is shown using detailed two-dimensional kinematics as well as metallicity measurements for the…

2015 The Astrophysical Journal
eHST 6
Broad Balmer Wings in BA Hyper/Supergiants Distorted by Diffuse Interstellar Bands: Five Examples in the 30 Doradus Region from the VLT-FLAMES Tarantula Survey
DOI: 10.1088/0004-637X/809/2/109 Bibcode: 2015ApJ...809..109W

Walborn, Nolan R.; Sana, Hugues; Ulaczyk, Krzysztof +11 more

Extremely broad emission wings at Hβ and Hα have been found in VLT-FLAMES Tarantula Survey data for five very luminous BA supergiants in or near 30 Doradus in the Large Magellanic Cloud. The profiles of both lines are extremely asymmetrical, which we have found to be caused by very broad diffuse interstellar bands (DIBs) in the longward wing of Hβ…

2015 The Astrophysical Journal
eHST 6
Unbiased Correction Relations for Galaxy Cluster Properties Derived from Chandra and XMM-Newton
DOI: 10.1088/0004-637X/799/1/47 Bibcode: 2015ApJ...799...47Z

Zhao, Hai-Hui; Jia, Shu-Mei; Chen, Yong +2 more

We use a sample of 62 clusters of galaxies to investigate the discrepancies between the gas temperature and total mass within r 500 from XMM-Newton and Chandra data. Comparisons of the properties show that (1) both the de-projected and projected temperatures determined by Chandra are higher than those of XMM-Newton and there is a good l…

2015 The Astrophysical Journal
XMM-Newton 6
Searching for Overionized Plasma in the Gamma-ray-emitting Supernova Remnant G349.7+0.2
DOI: 10.1088/0004-637X/804/2/124 Bibcode: 2015ApJ...804..124E

Ercan, E. N.; Majumdar, P.; Saha, L. +3 more

G349.7+0.2 is a supernova remnant (SNR) expanding in a dense medium of molecular clouds and interacting with clumps of molecular material emitting gamma-rays. We analyzed the gamma-ray data of the Large Area Telescope on board the Fermi Gamma-Ray Space Telescope and detected G349.7+0.2 in the energy range of 0.2-300 GeV with a significance of ∼13σ…

2015 The Astrophysical Journal
Suzaku 6
Detection of Flux Emergence, Splitting, Merging, and Cancellation of Network Fields. II. Apparent Unipolar Flux Change and Cancellation
DOI: 10.1088/0004-637X/814/2/134 Bibcode: 2015ApJ...814..134I

Hagenaar, H. J.; Iida, Y.; Yokoyama, T.

In this second paper in the series, we investigate occurrence frequencies of apparent unipolar processes, cancellation, and emergence of patch structures in quiet regions. Apparent unipolar events are considerably more frequent than cancellation and emergence, per our definition, which is consistent with Lamb et al. Furthermore, we investigate the…

2015 The Astrophysical Journal
Hinode SOHO 6
Recent Stellar Mass Assembly of Low-mass Star-forming Galaxies at Redshifts 0.3 < z < 0.9
DOI: 10.1088/0004-637X/799/1/36 Bibcode: 2015ApJ...799...36R

Barro, Guillermo; Tresse, Laurence; Charlot, Stéphane +5 more

The epoch when low-mass star-forming galaxies (LMSFGs) form the bulk of their stellar mass is uncertain. While some models predict an early formation, others favor a delayed scenario until later ages of the universe. We present constraints on the star formation histories (SFHs) of a sample of LMSFGs obtained through the analysis of their spectral …

2015 The Astrophysical Journal
eHST 6
The Kinematic and Chemical Properties of a Potential Core-forming Clump: Perseus B1-E
DOI: 10.1088/0004-637X/806/1/38 Bibcode: 2015ApJ...806...38S

André, Ph.; Henning, Th.; Di Francesco, J. +4 more

We present 13CO and {{C}18}O (1-0), (2-1), and (3-2) maps toward the core-forming Perseus B1-E clump using observations from the James Clerk Maxwell Telescope, the Submillimeter Telescope of the Arizona Radio Observatory, and the IRAM 30 m telescope. We find that the 13CO and {{C}18}O line emission both …

2015 The Astrophysical Journal
Herschel 6
Exploring the Bridge between A3556 and A3558 in the Shapley Supercluster
DOI: 10.1088/0004-637X/806/2/211 Bibcode: 2015ApJ...806..211U

Kelley, R. L.; Gupta, A.; Mitsuishi, I. +4 more

Looking at the region connecting two clusters is a promising way to identify and study the Warm-Hot Intergalactic Medium. Observations show that the spectrum of the bridge between A3556 and A3558 has a stronger soft X-ray emission than the nearby region. Suzaku observations could not discriminate the origin of the extra emission. In this work we a…

2015 The Astrophysical Journal
Suzaku 6
The Molecular H2 Emission and the Stellar Kinematics in the Nuclear Region of the Sombrero Galaxy
DOI: 10.1088/0004-637X/808/1/27 Bibcode: 2015ApJ...808...27M

Steiner, J. E.; Menezes, R. B.

We analyze the molecular H2 emission and the stellar kinematics in a data cube of the nuclear region of M104, the Sombrero galaxy, obtained with NIFS on the Gemini-north telescope. After a careful subtraction of the stellar continuum, the only emission line we detected in the data cube was {{{H}}}2λ 21218. An analysis of this…

2015 The Astrophysical Journal
eHST 5
Solar Micro-Type III Burst Storms and Long Dipolar Magnetic Field in the Outer Corona
DOI: 10.1088/0004-637X/808/2/191 Bibcode: 2015ApJ...808..191M

Misawa, H.; Kasaba, Y.; Miyoshi, Y. +4 more

Solar micro-type III radio bursts are elements of the so-called type III storms and are characterized by short-lived, continuous, and weak emissions. Their frequency of occurrence with respect to radiation power is quite different from that of ordinary type III bursts, suggesting that the generation process is not flare-related, but due to some re…

2015 The Astrophysical Journal
PROBA-2 SOHO 5