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12473133
1607.01526
Globular clusters as tracers of the host galaxy mass distribution: the Fornax dSph test case
The Fornax dwarf spheroidal galaxy is the most massive satellites of the Milky Way, claimed to be embedded in a huge dark matter halo, and the only among the Milky Way satellites hosting five globular clusters. Interestingly, their estimated masses, ages and positions seem hardly compatible with the presence of a signi...
[ 0.010727103799581528, 0.03195144236087799, 0.05062171071767807, 0.006477765738964081, 0.016077885404229164, 0.031976982951164246, 0.012336169369518757, -0.01306407991796732, -0.006608661729842424, 0.006825758144259453, -0.004217411857098341, -0.002841405337676406, -0.08045327663421631, -0....
9.992026
7.407736
2016-07-01
17
2016MNRAS.461.4335A
[ "cuspy density profiles", "dynamical friction", "Fornax GC", "Fornax", "the Fornax dark matter content", "five globular clusters", "the globular clusters", "direct N-body simulations", "the Fornax GC system", "a huge dark matter halo", "a standard density profile", "the Milky Way satellites", ...
[ "methods: numerical", "galaxies: individual: Fornax", "galaxies: nuclei", "galaxies: star clusters: general", "Astrophysics - Astrophysics of Galaxies" ]
1
[ "10.1093/mnras/stw1647", "10.48550/arXiv.1607.01526" ]
[ "Arca-Sedda, M.", "Capuzzo-Dolcetta, R." ]
[ "Department of Physics, Sapienza, University of Rome, Piazzale Aldo Moro 5, I-00185 Rome, Italy", "Department of Physics, Sapienza, University of Rome, Piazzale Aldo Moro 5, I-00185 Rome, Italy" ]
[ "2017MNRAS.464.3060A", "2017MNRAS.471..478A", "2018A&A...615A..91B", "2018MNRAS.477..480Z", "2018MNRAS.477.4423A", "2018MNRAS.479..900A", "2018MNRAS.480..927P", "2019ApJ...877..133D", "2019MNRAS.485.2546B", "2019MNRAS.488.2977O", "2020MNRAS.493..320L", "2020arXiv200906133A", "2021MNRAS.503.....
[ "1911MNRAS..71..460P", "1943ApJ....97..255C", "1975PASJ...27..533M", "1976ApJ...203...72T", "1977MNRAS.181..735B", "1983ApJ...270..365M", "1989MNRAS.241..849O", "1990ApJ...356..359H", "1991RMxAA..22..255A", "1992MNRAS.254..466P", "1994ApJ...427L...1F", "1994Natur.370..629M", "1996ApJ...462.....
5209849
1607.03009
Impacts of fragmented accretion streams onto classical T Tauri stars: UV and X-ray emission lines
Context. The accretion process in classical T Tauri stars (CTTSs) can be studied through the analysis of some UV and X-ray emission lines which trace hot gas flows and act as diagnostics of the post-shock downfalling plasma. In the UV-band, where higher spectral resolution is available, these lines are characterized by...
[ 0.010496567003428936, 0.033573903143405914, 0.015439461916685104, 0.005065680015832186, -0.010483973659574986, 0.0408276803791523, 0.030828550457954407, -0.03624369576573372, -0.007530830334872007, 0.03259161859750748, 0.006060555577278137, 0.011592189781367779, -0.007348226848989725, -0.0...
9.33351
12.213435
2016-07-01
15
2016A&A...594A..93C
[ "line profiles", "C IV line", "stream fragmentation", "O VIII lines", "accretion rates", "UV and X-ray emission lines", "dense blobs", "the post-shock downfalling plasma", "C IV doublet", "C IV", "fragmentation", "speed", "shocked upflows", "impact regions", "several plasma components", ...
[ "accretion", "accretion disks", "magnetohydrodynamics (MHD)", "stars: pre-main sequence", "shock waves", "X-rays: stars", "ultraviolet: stars", "Astrophysics - Solar and Stellar Astrophysics" ]
3
[ "10.1051/0004-6361/201628858", "10.48550/arXiv.1607.03009" ]
[ "Colombo, S.", "Orlando, S.", "Peres, G.", "Argiroffi, C.", "Reale, F." ]
[ "INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134, Palermo, Italy", "INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134, Palermo, Italy", "INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134, Palermo, Italy; Dipartimento di Fisica & Chimica,...
[ "2017A&A...598L...8P", "2017A&A...602A..10G", "2017A&A...607A..14A", "2017SciA....3E0982R", "2018MNRAS.475.4367D", "2019A&A...624A..50C", "2019A&A...629L...9C", "2019A&A...630A..84D", "2019ASPC..519...21I", "2019ASSP...55...29D", "2019ASSP...55...43O", "2019arXiv190409156D", "2020A&A...640A....
[ "1962pfig.book.....S", "1977ApJ...211..135C", "1984ApJ...277..605G", "1988ApJ...330..350B", "1991ApJ...370L..39K", "1993ApJ...404..625D", "1996JGR...10124443O", "1999JCoPh.149..270B", "2002ApJ...567..434K", "2007A&A...465L...5A", "2007ApJS..170..228M", "2008A&A...491L..17S", "2008MNRAS.388.....
12586989
1607.06240
Hybrid entropy stable HLL-type Riemann solvers for hyperbolic conservation laws
It is known that HLL-type schemes are more dissipative than schemes based on characteristic decompositions. However, HLL-type methods offer greater flexibility to large systems of hyperbolic conservation laws because the eigenstructure of the flux Jacobian is not needed. We demonstrate in the present work that several ...
[ 0.019672680646181107, 0.007757165934890509, 0.026120029389858246, 0.014471565373241901, 0.037132661789655685, 0.010453098453581333, -0.004317307844758034, -0.0019059102050960064, 0.03242749720811844, -0.017307382076978683, -0.021936247125267982, -0.016951315104961395, -0.06297292560338974, ...
8.773089
4.468664
2016-07-01
7
2017JCoPh.330..566S
[ "hyperbolic conservation laws", "entropy stability", "characteristic decompositions", "standard dissipation terms", "less dissipation", "large systems", "Jacobian", "HLL", "greater flexibility", "dissipation", "several HLL-type Riemann solvers", "hybrid HLL-type methods", "HLL-type schemes",...
[ "Entropy stability", "Ideal magnetohydrodynamics", "HLL", "Riemann solver", "Discrete entropy inequality", "Mathematics - Numerical Analysis", "Astrophysics - Instrumentation and Methods for Astrophysics" ]
1
[ "10.1016/j.jcp.2016.10.034", "10.48550/arXiv.1607.06240" ]
[ "Schmidtmann, Birte", "Winters, Andrew R." ]
[ "MathCCES, RWTH Aachen University, Schinkelstr. 2, 52062 Aachen, Germany", "Mathematisches Institut, Universitรคt zu Kรถln, Weyertal 86-90, 50931 Kรถln, Germany" ]
[ "2019JCoPh.378..477S", "2019ShWav..29..755P", "2020JCoPh.41609545T", "2021ApJS..257...24L", "2021ApJS..257...34F", "2022JCoPh.46811521W", "2023JCoPh.49312505H" ]
[ "1999CRASM.328..479D", "2003AcNum..12..451T", "2003JPlPh..69..253T", "2016JCoPh.304...72W", "2017SJSC...39A2911S" ]
168897
1607.07246
Dynamics of Saturnโ€™s great storm of 2010-2011 from Cassini ISS and RPWS
Saturnโ€™s quasi-periodic planet-encircling storms are the largest convecting cumulus outbursts in the Solar System. The last eruption was in 1990 (Sรกnchez-Lavega, A. [1994]. Chaos 4, 341-353). A new eruption started in December 2010 and presented the first-ever opportunity to observe such episodic storms from a spacecra...
[ 0.00915789045393467, -0.00003636578912846744, 0.02020278014242649, -0.0014622603775933385, -0.027447277680039406, 0.025415124371647835, -0.01141437329351902, -0.0368163026869297, 0.005773165728896856, 0.021667515859007835, 0.033227041363716125, 0.0304031390696764, -0.06571511924266815, -0....
8.500903
15.534467
2016-07-01
74
2013Icar..223..460S
[ "such episodic storms", "early August", "G. et al", "โˆผ40 days", "L.N. et al", "A. et al", "late August", "Plasma Wave Science", "SED", "Jupiter", "Saturn", "the SED radio signals", "motion", "demise", "latitudes", "Saturnโ€™s quasi-periodic planet-encircling storms", "RPWS", "-", "...
[ "Astrophysics - Earth and Planetary Astrophysics" ]
18
[ "10.1016/j.icarus.2012.12.013", "10.48550/arXiv.1607.07246" ]
[ "Sayanagi, Kunio M.", "Dyudina, Ulyana A.", "Ewald, Shawn P.", "Fischer, Georg", "Ingersoll, Andrew P.", "Kurth, William S.", "Muro, Gabriel D.", "Porco, Carolyn C.", "West, Robert A." ]
[ "Department of Atmospheric and Planetary Sciences, Hampton University, Hampton, VA 23668, USA; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA", "Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA", ...
[ "2013Icar..226..641L", "2013Icar..226.1020D", "2013JGRA..118.7246C", "2013PhFl...25f6604S", "2014AnGeo..32.1463F", "2014ApJ...786...92A", "2014Icar..229..170S", "2014Icar..238..110G", "2014Icar..241..313D", "2014Icar..242..122T", "2014MNRAS.444.1369H", "2014Natur.505..625S", "2015A&A...580A....
[ "1949JAtS....6..105K", "1973Icar...20..465W", "1982Natur.297..132H", "1982Sci...215..504S", "1983JGR....88.8650S", "1986Icar...65..335L", "1988JAtS...45.1380D", "1989NASSP.494..245B", "1989Sci...245.1367H", "1991Natur.353..397S", "1991Sci...254..684S", "1992Icar...95..163B", "1992Icar..100.....
12408831
1607.07888
Observed Variability at 1 and 4 ฮผm in the Y0 Brown Dwarf WISEP J173835.52+273258.9
We have monitored photometrically the Y0 brown dwarf WISEP J173835.52+273258.9 (W1738) at both near- and mid-infrared wavelengths. This โ‰ฒ1 Gyr old 400 K dwarf is at a distance of 8 pc and has a mass around 5 M <SUB>Jupiter</SUB>. We observed W1738 using two near-infrared filters at ฮป โ‰ˆ 1 ฮผm, Y and J, on Gemini Observat...
[ -0.052903518080711365, 0.04128861054778099, 0.017143921926617622, -0.009924381971359253, -0.04834241420030594, 0.009606165811419487, 0.07356108725070953, -0.022500569000840187, 0.0007648801547475159, 0.025284964591264725, -0.010302264243364334, -0.028453873470425606, -0.05038430541753769, ...
7.153717
12.541796
2016-07-01
31
2016ApJ...830..141L
[ "large features", "associated small changes", "surface temperature", "-infrared wavelengths", "significant evolution", "patchy KCl", "atmospheric models", "Jupiter</SUB", "variability", "evolution", "The mid-infrared light curves", "the solar system gas giants", "a โˆผ3.0 hr period", "Gemini...
[ "brown dwarfs", "stars: atmospheres", "stars: individual: WISEP J173835.52+273258.9", "Astrophysics - Solar and Stellar Astrophysics" ]
10
[ "10.3847/0004-637X/830/2/141", "10.48550/arXiv.1607.07888" ]
[ "Leggett, S. K.", "Cushing, Michael C.", "Hardegree-Ullman, Kevin K.", "Trucks, Jesica L.", "Marley, M. S.", "Morley, Caroline V.", "Saumon, D.", "Carey, S. J.", "Fortney, J. J.", "Gelino, C. R.", "Gizis, J. E.", "Kirkpatrick, J. D.", "Mace, G. N." ]
[ "Gemini Observatory, Northern Operations Center, 670 N. A'ohoku Place, Hilo, HI 96720, USA", "The University of Toledo, 2801 West Bancroft Street, Mailstop 111, Toledo, OH 43606, USA", "The University of Toledo, 2801 West Bancroft Street, Mailstop 111, Toledo, OH 43606, USA", "The University of Toledo, 2801 W...
[ "2016ApJ...832...58E", "2017ApJ...842...78V", "2017ApJ...842..118L", "2017MNRAS.468.3764S", "2017arXiv170802821A", "2018AJ....155..238S", "2018ApJ...867...96L", "2018ApJ...867..109M", "2018haex.bookE..94A", "2019A&A...629A.145E", "2019ApJ...874..111T", "2019ApJ...875L..15M", "2019ApJ...877.....
[ "1989AJ.....98.2268H", "1997ApJ...491..856B", "2000ASPC..212.....G", "2003AJ....126..348T", "2003AJ....126.1006E", "2003ApJ...596..587B", "2003PASP..115.1388H", "2004ApJS..154...10F", "2008A&A...487..277G", "2008ApJ...689.1327S", "2009ApJ...701.1534A", "2010ApJ...710.1142B", "2010arXiv1008.4...
12518466
1607.08820
"Dispersion by pulsars, magnetars, fast radio bursts and massive electromagnetism at very low radio (...TRUNCATED)
"Our understanding of the universe relies mostly on electromagnetism. As photons are the messengers,(...TRUNCATED)
[-0.00632535619661212,0.011160125955939293,0.012271640822291374,0.01770714297890663,0.00273381313309(...TRUNCATED)
6.522832
3.614386
2016-07-01
28
2017AdSpR..59..736B
["unknown origin","pulsar observations","Radio astronomy","OLFAR","observations","low frequencies","(...TRUNCATED)
["Photons","Radio astronomy","Satellites","Pulsars","Magnetars","Fast radio bursts","Astrophysics - (...TRUNCATED)
6
[ "10.1016/j.asr.2016.10.018", "10.48550/arXiv.1607.08820" ]
[ "Bentum, Mark J.", "Bonetti, Luca", "Spallicci, Alessandro D. A. M." ]
["Universiteit van Twente, Faculteit van Elektrotechniek, Wiskunde en Informatica, Telecommunication(...TRUNCATED)
["2017ApJ...842...23Y","2017CQGra..34u5006S","2017FoPh...47..769A","2017PhLB..764..203B","2017PhLB..(...TRUNCATED)
["1933PhRv...44..855H","1934PhRv...46.1087B","1934RSPSA.144..425B","1936AnP...418..398E","1936ZPhy..(...TRUNCATED)
12406228
1607.06710
"Setting the volatile composition of (exo)planet-building material. Does chemical evolution in disk (...TRUNCATED)
"Context. The atmospheres of extrasolar planets are thought to be built largely through accretion of(...TRUNCATED)
[0.008736980147659779,0.01737302727997303,0.059953976422548294,0.0015250288415700197,-0.003882751800(...TRUNCATED)
10.068603
13.044076
2016-07-01
146
2016A&A...595A..83E
["SUB>2</SUB","interstellar ice abundances","grain surfaces","CO","initial abundances","ices","atomi(...TRUNCATED)
["astrochemistry","planets and satellites: formation","protoplanetary disks","planets and satellites(...TRUNCATED)
12
[ "10.1051/0004-6361/201628509", "10.48550/arXiv.1607.06710" ]
[ "Eistrup, Christian", "Walsh, Catherine", "van Dishoeck, Ewine F." ]
["Leiden Observatory, Leiden University, PO Box 9513, 2300 RA, Leiden, The Netherlands","Leiden Obse(...TRUNCATED)
["2017A&A...599A.101V","2017A&A...599A.113M","2017A&A...601A..36B","2017A&A...603A.123H","2017A&A...(...TRUNCATED)
["1972GeCoA..36..597G","1977Ap&SS..51..153W","1982A&A...114..245T","1983ApJ...267..603P","1993MNRAS.(...TRUNCATED)
2774767
1607.08619
The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey
"Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) is an optical fiber-bundle integral-fie(...TRUNCATED)
[-0.018747791647911072,0.03372214362025261,0.015452002175152302,-0.010926260612905025,-0.02956658229(...TRUNCATED)
11.558285
6.853098
2016-07-01
359
2016AJ....152...83L
["Sloan Digital Sky Survey","MaNGA","individual dithered observations","SDSS-IV Data Release","centr(...TRUNCATED)
["methods: data analysis","surveys","techniques: imaging spectroscopy","Astrophysics - Instrumentati(...TRUNCATED)
32
[ "10.3847/0004-6256/152/4/83", "10.48550/arXiv.1607.08619" ]
["Law, David R.","Cherinka, Brian","Yan, Renbin","Andrews, Brett H.","Bershady, Matthew A.","Bizyaev(...TRUNCATED)
["Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA","Center for As(...TRUNCATED)
["2016AJ....152..197Y","2016MNRAS.463.2513B","2017AJ....154...28B","2017ApJ...837...32L","2017ApJ...(...TRUNCATED)
["1969PASP...81..527W","1982PASP...94..715F","1986PASP...98..609H","1996PASP..108..277O","1998ApJ...(...TRUNCATED)
12585901
1607.08157
Dark matter directional detection: comparison of the track direction determination
"Several directional techniques have been proposed for a directional detection of Dark matter, among(...TRUNCATED)
[0.011932607740163803,0.024745754897594452,0.01089667808264494,0.027581609785556793,-0.0341079644858(...TRUNCATED)
7.520985
-2.487568
2016-07-01
10
2017JCAP...01..027C
["initial direction","different detector materials","crystal detectors","nuclear emulsion plates","W(...TRUNCATED)
["Astrophysics - Instrumentation and Methods for Astrophysics","Physics - Instrumentation and Detect(...TRUNCATED)
3
[ "10.1088/1475-7516/2017/01/027", "10.48550/arXiv.1607.08157" ]
[ "Couturier, C.", "Zopounidis, J. P.", "Sauzet, N.", "Naraghi, F.", "Santos, D." ]
["LPSC, CNRS/IN2P3, UJF, INP, Avenue des Martyrs, 38000, Grenoble, France","LPSC, CNRS/IN2P3, UJF, I(...TRUNCATED)
["2016arXiv160708765C","2017JInst..12P0009B","2017PhRvD..96h3011O","2020PhRvD.102g5036B","2020PhRvD.(...TRUNCATED)
["1985PhRvD..31.3059G","1988PhRvD..37.1353S","2003PhLB..571..132S","2010NIMPB.268.1818Z","2012EAS...(...TRUNCATED)
12509827
1607.01847
Oscillating chiral tensor spectrum from axionic inflation
"We study axionic inflation with a modulated potential and examine if the primordial tensor power sp(...TRUNCATED)
[0.018994921818375587,0.023814870044589043,-0.02079528011381626,-0.005090570542961359,-0.01004440523(...TRUNCATED)
10.62901
-1.476708
2016-07-01
42
2016PhRvD..94d4062O
["chiral gravitational waves","axion phenomenologies","BBO","single-field axion monodromy inflation"(...TRUNCATED)
["Astrophysics - Cosmology and Nongalactic Astrophysics","General Relativity and Quantum Cosmology",(...TRUNCATED)
6
[ "10.1103/PhysRevD.94.044062", "10.48550/arXiv.1607.01847" ]
[ "Obata, Ippei", "Soda, Jiro" ]
["Department of Physics, Kyoto University, Kyoto 606-8502, Japan","Department of Physics, Kobe Unive(...TRUNCATED)
["2016JCAP...12..031G","2016JHEP...12..137A","2017JCAP...06..050O","2017JCAP...08..005G","2017JHEP..(...TRUNCATED)
["1990PhRvL..65.3233F","1998PhRvD..57.7089C","2000PhR...331..283M","2001PhRvL..87v1103S","2005IJMPD.(...TRUNCATED)
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