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Constraining holographic cosmology using Planck data
DOI: 10.1103/PhysRevD.95.123505 Bibcode: 2017PhRvD..95l3505A

Afshordi, Niayesh; Gould, Elizabeth; Skenderis, Kostas

Holographic cosmology offers a novel framework for describing the very early Universe in which cosmological predictions are expressed in terms of the observables of a three-dimensional quantum field theory (QFT). This framework includes conventional slow-roll inflation, which is described in terms of a strongly coupled QFT, but it also allows for …

2017 Physical Review D
Planck 22
Multi-wavelength Spectral Analysis of Ellerman Bombs Observed by FISS and IRIS
DOI: 10.3847/1538-4357/aa671e Bibcode: 2017ApJ...838..101H

Cao, Wenda; Ding, M. D.; Hong, Jie

Ellerman bombs (EBs) are a kind of solar activity that is suggested to occur in the lower solar atmosphere. Recent observations using the Interface Region Imaging Spectrograph (IRIS) show connections between EBs and IRIS bombs (IBs), which imply that EBs might be heated to a much higher temperature (8 × 104 K) than previous results. Her…

2017 The Astrophysical Journal
IRIS 22
Absolute-magnitude Calibration for W UMa-type Systems Based on Gaia Data
DOI: 10.3847/1538-3881/aa8453 Bibcode: 2017AJ....154..125M

Rucinski, Slavek M.; Mateo, Nicole M.

Tycho-Gaia Astrometric Solution (TGAS) parallax data are used to determine absolute magnitudes M V for 318 W UMa-type (EW) contact binary stars. A very steep (slope ≃ -9), single-parameter ({log}P), linear calibration can be used to predict M V to about 0.1-0.3 mag over the whole range of accessible orbital period, 0.22&l…

2017 The Astronomical Journal
Gaia 22
Observational Constraints on Correlated Star Formation and Active Galactic Nuclei in Late-stage Galaxy Mergers
DOI: 10.3847/1538-4357/aa93de Bibcode: 2017ApJ...850...27B

Zakamska, Nadia L.; Comerford, Julia M.; Barrows, R. Scott +1 more

Galaxy mergers are capable of triggering both star formation and active galactic nuclei (AGNs) and therefore may represent an important pathway in the co-evolution of galaxies and supermassive black holes (SMBHs). However, correlated enhancements of merger-induced star formation and AGN triggering may be hidden by the variable conditions and times…

2017 The Astrophysical Journal
eHST 22
Draining the Local Void
DOI: 10.3847/1538-4357/835/1/78 Bibcode: 2017ApJ...835...78R

Shaya, Edward J.; Tully, R. Brent; Karachentsev, Igor D. +2 more

Two galaxies that lie deep within the Local Void provide a test of the expectation that voids expand. The modest ({M}B∼ -14) HI bearing dwarf galaxies ALFAZOAJ1952+1428 and KK246 have been imaged with Hubble Space Telescope in order to study the stellar populations and determine distances from the luminosities of stars at the tip of the…

2017 The Astrophysical Journal
eHST 22
A Nearly Naked Supermassive Black Hole
DOI: 10.3847/1538-4357/834/2/184 Bibcode: 2017ApJ...834..184C

Darling, Jeremy; Petrov, L.; Condon, J. J. +1 more

During a systematic search for supermassive black holes (SMBHs) not in galactic nuclei, we identified the compact, symmetric radio source B3 1715+425 with an emission-line galaxy offset ≈ 8.5 {kpc} from the nucleus of the brightest cluster galaxy (BCG) in the redshift z = 0.1754 cluster ZwCl 8193. B3 1715+425 is too bright (brightness temperature …

2017 The Astrophysical Journal
eHST 22
Hub-filament System in IRAS 05480+2545: Young Stellar Cluster and 6.7 GHz Methanol Maser
DOI: 10.3847/1538-4357/aa79a5 Bibcode: 2017ApJ...844...15D

Dewangan, L. K.; Ojha, D. K.; Baug, T.

To probe the star formation (SF) process, we present a multi-wavelength study of IRAS 05480+2545 (hereafter I05480+2545). Analysis of Herschel data reveals a massive clump (M clump ∼ 1875 {M}; peak N(H2) ∼ 4.8 × 1022 cm-2 A V ∼ 51 mag) containing the 6.7 GHz methanol maser and I…

2017 The Astrophysical Journal
Herschel 22
Cassini ISS observation of Saturn's north polar vortex and comparison to the south polar vortex
DOI: 10.1016/j.icarus.2016.12.011 Bibcode: 2017Icar..285...68S

Dyudina, Ulyana A.; Ingersoll, Andrew P.; Ewald, Shawn P. +2 more

We present analyses of Saturn's north pole using high-resolution images captured in late 2012 by the Cassini spacecraft's Imaging Science Subsystem (ISS) camera. The images reveal the presence of an intense cyclonic vortex centered at the north pole. In the red and green visible continuum wavelengths, the north polar region exhibits a cyclonically…

2017 Icarus
Cassini 22
Neptune long-lived atmospheric features in 2013-2015 from small (28-cm) to large (10-m) telescopes
DOI: 10.1016/j.icarus.2017.06.009 Bibcode: 2017Icar..295...89H

Hueso, R.; Sánchez-Lavega, A.; Rojas, J. F. +32 more

Since 2013, observations of Neptune with small telescopes (28-50 cm) have resulted in several detections of long-lived bright atmospheric features that have also been observed by large telescopes such as Keck II or Hubble. The combination of both types of images allows the study of the long-term evolution of major cloud systems in the planet. In 2…

2017 Icarus
eHST 22
Distances of cataclysmic variables and related objects derived from Gaia Data Release 1
DOI: 10.1051/0004-6361/201730679 Bibcode: 2017A&A...604A.107R

Ramsay, Gavin; Wheatley, Peter J.; Gänsicke, Boris T. +1 more

We consider the parallaxes of sixteen cataclysmic variables and related objects that are included in the TGAS catalogue, which is part of the Gaia first data release, and compared these with previous parallax measurements. The parallax of the dwarf nova SS Cyg is consistent with the parallax determination made using the VLBI, but with only one of …

2017 Astronomy and Astrophysics
Gaia 22