Search Publications

Reconstruction of constant slow-roll inflation
DOI: 10.1007/s11433-017-9065-4 Bibcode: 2017SCPMA..60i0411G

Gao, Qing

Using the relations between the slow-roll parameters and the power spectra for the single field slow-roll inflation, we derive the scalar spectral tilt n s and the tensor to scalar ratio r for the constant slow-roll inflation, and obtain the constraint on the slow-roll parameter η from the Planck 2015 results. The inflationary potenti…

2017 Science China Physics, Mechanics, and Astronomy
Planck 34
Far-infrared observations of a massive cluster forming in the Monoceros R2 filament hub
DOI: 10.1051/0004-6361/201630039 Bibcode: 2017A&A...607A..22R

Bernard, J. -P.; Hill, T.; White, G. J. +29 more

We present far-infrared observations of Monoceros R2 (a giant molecular cloud at approximately 830 pc distance, containing several sites of active star formation), as observed at 70 µm, 160 µm, 250 µm, 350 µm, and 500 µm by the Photodetector Array Camera and Spectrometer (PACS) and Spectral and Photometric Imaging Rec…

2017 Astronomy and Astrophysics
Herschel 34
Star Formation at z = 2.481 in the Lensed Galaxy SDSS J1110 = 6459. I. Lens Modeling and Source Reconstruction
DOI: 10.3847/1538-4357/aa7756 Bibcode: 2017ApJ...843...78J

Rigby, Jane R.; Florian, Michael; Whitaker, Katherine E. +6 more

Using the combined resolving power of the Hubble Space Telescope and gravitational lensing, we resolve star-forming structures in a z∼ 2.5 galaxy on scales much smaller than the usual kiloparsec diffraction limit of HST. SGAS J111020.0+645950.8 is a clumpy, star-forming galaxy lensed by the galaxy cluster SDSS J1110+6459 at z=0.659, with a total m…

2017 The Astrophysical Journal
eHST 34
The highly active Anhur-Bes regions in the 67P/Churyumov-Gerasimenko comet: results from OSIRIS/ROSETTA observations
DOI: 10.1093/mnras/stx1275 Bibcode: 2017MNRAS.469S..93F

Jorda, L.; Lamy, P. L.; Bertaux, J. -L. +51 more

The Southern hemisphere of the 67P/Churyumov-Gerasimenko comet has become visible from Rosetta only since 2015 March. It was illuminated during the perihelion passage and therefore it contains the regions that experienced the strongest heating and erosion rates, thus exposing the sub-surface most pristine material. In this work we investigate, tha…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 34
The “UV-route” to Search for Blue Straggler Stars in Globular Clusters: First Results from the HST UV Legacy Survey
DOI: 10.3847/1538-4357/aa6891 Bibcode: 2017ApJ...839...64R

Dalessandro, E.; Nardiello, D.; Vesperini, E. +4 more

We used data from the Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters to select the Blue Straggler Star (BSS) population in four intermediate/high density systems (namely NGC 2808, NGC 6388, NGC 6541, and NGC 7078) through a “UV-guided search.” This procedure consists of using the F275W images in each cluster to construct the…

2017 The Astrophysical Journal
eHST 34
Importance of CME Radial Expansion on the Ability of Slow CMEs to Drive Shocks
DOI: 10.3847/1538-4357/aa8ef9 Bibcode: 2017ApJ...848...75L

Lugaz, Noé; Farrugia, Charles J.; Winslow, Reka M. +3 more

Coronal mass ejections (CMEs) may disturb the solar wind by overtaking it or expanding into it, or both. CMEs whose front moves faster in the solar wind frame than the fast magnetosonic speed drive shocks. Such shocks are important contributors to space weather, by triggering substorms, compressing the magnetosphere, and accelerating particles. In…

2017 The Astrophysical Journal
SOHO 34
Exploring the Inner Acceleration Region of Solar Wind: A Study Based on Coronagraphic UV and Visible Light Data
DOI: 10.3847/1538-4357/aa7de4 Bibcode: 2017ApJ...846...86B

Bemporad, A.

This work combined coronagraphic visible light (VL) and UV data to provide with an unprecedented view of the inner corona where the nascent solar wind is accelerated. The UV (H I Lyα) and VL (polarized brightness) images (reconstructed with SOHO/UVCS, LASCO, and Mauna Loa data) have been analyzed with the Doppler dimming technique to provide for t…

2017 The Astrophysical Journal
SOHO 34
Specific Frequencies and Luminosity Profiles of Cluster Galaxies and Intracluster Light in Abell 1689
DOI: 10.3847/1538-4357/aa8f44 Bibcode: 2017ApJ...849....6A

Blakeslee, J. P.; Alamo-Martínez, K. A.

We present magnitudes and profile fits for 180 galaxies in the central field of the massive lensing cluster Abell 1689 using very deep imaging with the Hubble Space Telescope Advanced Camera for Surveys in the F814W bandpass. Previous work revealed an exceptionally large number of globular clusters (GCs) in A1689 and mapped their number density di…

2017 The Astrophysical Journal
eHST 34
Photometric Determination of the Mass Accretion Rates of Pre-main-sequence Stars. V. Recent Star Formation in the 30 Dor Nebula
DOI: 10.3847/1538-4357/aa85e9 Bibcode: 2017ApJ...846..110D

Panagia, Nino; Beccari, Giacomo; De Marchi, Guido

We report on the properties of the low-mass stars that recently formed in the central ∼ 2\buildrel{ \prime}\over{.} 7× 2\buildrel{ \prime}\over{.} 7 of 30 Dor, including the R136 cluster. Using the photometric catalog of De Marchi et al., based on observations with the Hubble Space Telescope, and the most recent extinction law for this field, we i…

2017 The Astrophysical Journal
eHST 34
Traveling Foreshocks and Transient Foreshock Phenomena
DOI: 10.1002/2017JA023901 Bibcode: 2017JGRA..122.9148K

Omidi, N.; Blanco-Cano, X.; Kajdič, P. +3 more

We use the multispacecraft capabilities of the Cluster and Time History of Events and Macroscale Interactions during Substorms (THEMIS) missions to show that two types of foreshock may be detected in spacecraft data. One is the global foreshock that appears upstream of the Earth's quasi-parallel bow shock under steady or variable interplanetary ma…

2017 Journal of Geophysical Research (Space Physics)
Cluster 34