Search Publications

Geomorphology and spectrophotometry of Philae's landing site on comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201525983 Bibcode: 2015A&A...583A..41L

Jorda, L.; Bertaux, J. -L.; Lamy, P. +52 more

Context. On 12 November 2014 the European mission Rosetta succeeded in delivering a lander, named Philae, on the surface of one of the smallest, low-gravity and most primitive bodies of the solar system, the comet 67P/Churyumov-Gerasimenko (67P).
Aims: The aim of this paper is to provide a comprehensive geomorphological and spectrophotometric…

2015 Astronomy and Astrophysics
Rosetta 42
Non-conservative evolution in Algols: where is the matter?
DOI: 10.1051/0004-6361/201424772 Bibcode: 2015A&A...577A..55D

Baes, M.; Jorissen, A.; Siess, L. +3 more

Context. There is indirect evidence of non-conservative evolutions in Algols. However, the systemic mass-loss rate is poorly constrained by observations and generally set as a free parameter in binary-star evolution simulations. Moreover, systemic mass loss may lead to observational signatures that still need to be found.
Aims: Within the "ho…

2015 Astronomy and Astrophysics
IUE eHST 42
Stellar cycles from photometric data: CoRoT stars
DOI: 10.1051/0004-6361/201424900 Bibcode: 2015A&A...583A.134F

Catelan, M.; Ferreira Lopes, C. E.; De Medeiros, J. R. +3 more

Context. Until a few years ago, the amplitude variation in the photometric data had been explored to a limited extent mainly because of time resolution and photometric sensitivity limitations. This investigation is now possible thanks to the Kepler and CoRoT databases which provide a unique set of data for studying the nature of stellar variabilit…

2015 Astronomy and Astrophysics
CoRoT 42
Outflow of low-energy ions and the solar cycle
DOI: 10.1002/2014JA020714 Bibcode: 2015JGRA..120.1072A

André, M.; Eriksson, A. I.; Li, K.

Magnetospheric ions with energies less than tens of eV originate from the ionosphere. Positive low-energy ions are complicated to detect onboard sunlit spacecraft at higher altitudes, which often become positively charged to several tens of volts. We use two Cluster spacecraft and study low-energy ions with a technique based on the detection of th…

2015 Journal of Geophysical Research (Space Physics)
Cluster 42
Overturning the Case for Gravitational Powering in the Prototypical Cooling Lyα Nebula
DOI: 10.1088/0004-637X/802/1/32 Bibcode: 2015ApJ...802...32P

Momcheva, Ivelina; Brammer, Gabriel B.; Fynbo, Johan P. U. +2 more

The Nilsson et al. Lyα nebula has often been cited as the most plausible example of an Lyα nebula powered by gravitational cooling. In this paper, we bring together new data from the Hubble Space Telescope and the Herschel Space Observatory as well as comparisons to recent theoretical simulations in order to revisit the questions of the local envi…

2015 The Astrophysical Journal
Herschel eHST 42
The Host Galaxies of X-Ray Quasars are Not Strong Star Formers
DOI: 10.1088/0004-637X/801/2/87 Bibcode: 2015ApJ...801...87B

Hasinger, G.; Li, Y.; Owen, F. N. +4 more

We use ultradeep SCUBA-2 850 µm observations (∼0.37 mJy rms) of the 2 Ms Chandra Deep Field-North (CDF-N) and 4 Ms Chandra Deep Field-South X-ray fields to examine the amount of dusty star formation taking place in the host galaxies of high-redshift X-ray active galactic nuclei (AGNs). Supplementing with COSMOS, we measure the submillimeter …

2015 The Astrophysical Journal
Herschel eHST 42
A Connection between Plasma Conditions near Black Hole Event Horizons and Outflow Properties
DOI: 10.1088/0004-637X/814/2/139 Bibcode: 2015ApJ...814..139K

Gandhi, P.; Bernardini, F.; Casella, P. +9 more

Accreting black holes are responsible for producing the fastest, most powerful outflows of matter in the universe. The formation process of powerful jets close to black holes is poorly understood, and the conditions leading to jet formation are currently hotly debated. In this paper, we report an unambiguous empirical correlation between the prope…

2015 The Astrophysical Journal
eHST 42
Deep NuSTAR and Swift Monitoring Observations of the Magnetar 1E 1841-045
DOI: 10.1088/0004-637X/807/1/93 Bibcode: 2015ApJ...807...93A

An, Hongjun; Hailey, Charles J.; Kaspi, Victoria M. +15 more

We report on a 350 ks NuSTAR observation of the magnetar 1E 1841-045 taken in 2013 September. During the observation, NuSTAR detected six bursts of short duration, with T90 ≲ 1 s. An elevated level of emission tail is detected after the brightest burst, persisting for ∼1 ks. The emission showed a power-law decay with a temporal index of…

2015 The Astrophysical Journal
XMM-Newton 42
ALMA observations of α Centauri. First detection of main-sequence stars at 3 mm wavelength
DOI: 10.1051/0004-6361/201425189 Bibcode: 2015A&A...573L...4L

Olofsson, G.; Eiroa, C.; Marshall, J. P. +19 more

Context. The precise mechanisms that provide the non-radiative energy for heating the chromosphere and the corona of the Sun and those of other stars constitute an active field of research. By studying stellar chromospheres one aims at identifying the relevant physical processes. Defining the permittable extent of the parameter space can also serv…

2015 Astronomy and Astrophysics
Herschel 42
Debris Distribution in HD 95086—A Young Analog of HR 8799
DOI: 10.1088/0004-637X/799/2/146 Bibcode: 2015ApJ...799..146S

Rieke, George H.; Su, Kate Y. L.; Malhotra, Renu +3 more

HD 95086 is a young early-type star that hosts (1) a 5 MJ planet at the projected distance of 56 AU revealed by direct imaging, and (2) a prominent debris disk. Here we report the detection of 69 µm crystalline olivine feature from the disk using the Spitzer/MIPS-SED data covering 55-95 µm. Due to the low resolution of the M…

2015 The Astrophysical Journal
Herschel 42