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Chandra and XMM ‑Newton: Synergies now and in the future
DOI: 10.1002/asna.201713321 Bibcode: 2017AN....338..140W

Wilkes, B. J.

2017 Astronomische Nachrichten
XMM-Newton 0
Compact star forming galaxies as the progenitors of compact quiescent galaxies: Clustering result
DOI: 10.1016/j.newast.2016.08.013 Bibcode: 2017NewA...51...99L

Fang, Guanwen; Kong, Xu; Fan, Lulu +1 more

We present a measurement of the spatial clustering of massive compact galaxies at 1.2 ≤ z ≤ 3 in CANDELS/3D-HST fields. We obtain the correlation length for compact quiescent galaxies (cQGs) at z ∼ 1.6 of r0 = 7.1-2.6+2.3 h-1 Mpc and compact star forming galaxies (cSFGs) at z ∼ 2.5 of r0 = 7.7…

2017 New Astronomy
eHST 0
Spectral Evolution of Novae in the Near-Infrared Based on Akari Observations
DOI: 10.5303/PKAS.2017.32.1.101 Bibcode: 2017PKAS...32..101S

Onaka, Takashi; Usui, Fumihiko; Matsuhara, Hideo +5 more

2017 Publication of Korean Astronomical Society
AKARI 0
The 5 Gyr evolution of sub-M* galaxies
DOI: 10.1093/mnras/stw3157 Bibcode: 2017MNRAS.466.2337D

Yang, Y.; Flores, H.; Hammer, F. +3 more

We gathered two complete samples of MAB(r) < -18 (Mstar > 109 M) galaxies, which are representative of the present-day galaxies and their counterparts at 5 Gyr ago. We analysed their 2D luminosity profiles and carefully decomposed them into bulges, bars and discs. This was done in a very consisten…

2017 Monthly Notices of the Royal Astronomical Society
eHST 0
X-ray observations of Galactic H.E.S.S. sources: An update
DOI: 10.1002/asna.201713342 Bibcode: 2017AN....338..274P

Pühlhofer, G.; Sasaki, M.; Eger, P. +3 more

X-ray diagnostics of TeV (teraelectronvolt) sources continues to be an important tool to identify the nature of newly detected sources as well as to pinpoint the physics processes that are at work in these highly energetic objects. This paper gives a review of recent studies that have been performed on TeV sources with H.E.S.S. and XMM-Newton and …

2017 Astronomische Nachrichten
XMM-Newton 0
Editorial: Comets: A new vision after Rosetta and Philae
DOI: 10.1093/mnras/stw3193 Bibcode: 2017MNRAS.469S...1T

Taylor, Matt G. G. T.

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 0
AKARI Infrared Camera Survey of the Large Magellanic Cloud
DOI: 10.5303/PKAS.2017.32.1.083 Bibcode: 2017PKAS...32...83S

Onaka, T.; Ita, Y.; Kato, D. +2 more

We conducted an unbiased near- to mid-infrared imaging and spectroscopic survey of the Large Magellanic Cloud (LMC) as a part of the AKARI Mission Program "Large-area Survey of the LMC" (LSLMC, PI: T. Onaka). An area of about 10 square degrees of the LMC was observed by five photometric bands (3.2, 7, 11, 15, and 24 µm) and a low-resolution …

2017 Publication of Korean Astronomical Society
AKARI 0
Dawn-Dusk Asymmetries of Ionospheric Outflow
DOI: 10.1002/9781119216346.ch21 Bibcode: 2017GMS...230..273L

Wei, Y.; Daly, P. W.; André, M. +3 more

2017 Dawn-Dusk Asymmetries in Planetary Plasma Environments
Cluster 0
Unveiling the physics of AGN through X-ray variability
Bibcode: 2017hsa9.conf..169H

González-Martín, O.; Márquez, I.; Masegosa, J. +1 more

Although variability is a general property characterizing active galactic nuclei (AGN), it is not well established whether the changes occur in the same way in every nuclei. The main purpose of this work is to study the X-ray variability pattern(s) in AGN selected at optical wavelengths in a large sample, including low ionization nuclear emission …

2017 Highlights on Spanish Astrophysics IX
XMM-Newton 0
IR photometry results and dust envelope model for symbiotic Mira star candidate V 335 Vul
DOI: 10.1134/S1990341317040071 Bibcode: 2017AstBu..72..447B

Bogdanov, M. B.; Taranova, O. G.; Shenavrin, V. I.

We present the results of JHKLM-photometry for the symbiotic Mira star candidate V 335 Vul. Based on the average flux data, supplemented by IRAS, MSX, AKARI, and WISE mid-IR observations, we calculated a model of a spherically symmetric dust envelope of the star, made up of amorphous carbon and silicon carbide particles. The optical depth of the e…

2017 Astrophysical Bulletin
AKARI 0