output
19962026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations

Showing 2014 · astro-ph.SRShow all

38 papers · 2 filters

astro-ph.SR2014★ 68 cited

The Chandra Planetary Nebulae Survey (ChanPlaNS): III. X-ray Emission from the Central Stars of Planetary Nebulae

R. Montez, J. H. Kastner, B. Balick +25

We present X-ray spectral analysis of 20 point-like X-ray sources detected in Chandra Planetary Nebula Survey (ChanPlaNS) observations of 59 planetary nebulae (PNe) in the solar ne…

astro-ph.SR2014★ 64 cited

Active-Region Tilt Angles: Magnetic Versus White-Light Determinations of Joy's Law

Y. -M. Wang, R. C. Colaninno, T. Baranyi +1

The axes of solar active regions are inclined relative to the east--west direction, with the tilt angle tending to increase with latitude ("Joy's law"). Observational determination…

astro-ph.SR2014★ 81 cited

Observations of Infalling and Rotational Motions on a 1,000-AU Scale around 17 Class 0 and 0/I Protostars: Hints of Disk Growth and Magnetic Braking?

Hsi-Wei Yen, Patrick M. Koch, Shigehisa Takakuwa +3

We perform imaging and analyses of SMA 1.3 mm continuum, C18O (2-1) and 12CO (2-1) line data of 17 Class 0 and 0/I protostars to study their gas kinematics on a 1,000-AU scale. Con…

astro-ph.SR2014★ 21 cited

HST Images Reveal Dramatic Changes in the Core of IRC+10216

Hyosun Kim, Ho-Gyu Lee, Nicolas Mauron +1

IRC+10216 is the nearest carbon star with a very high mass-loss rate. The existence of a binary companion has been hinted by indirect observational evidence, such as the bipolar mo…

astro-ph.SR2014★ 2 cited

The Identification of Extreme Asymptotic Giant Branch Stars and Red Supergiants in M33 by 24 μm Variability

Edward J. Montiel, Sundar Srinivasan, Geoffrey C. Clayton +2

We present the first detection of 24 μm variability in 24 sources in the Local Group galaxy M33. These results are based on 4 epochs of MIPS observations, which are irregularly spa…

astro-ph.SR2014★ 25 cited

The born-again planetary nebula A78: an X-ray twin of A30

J. A. Toalá, M. A. Guerrero, H. Todt +8

We present the XMM-Newton discovery of X-ray emission from the planetary nebula (PN) A78, the second born-again PN detected in X-rays apart from A30. These two PNe share similar sp…

astro-ph.SR2014★ 86 cited

The Structure of Pre-transitional Protoplanetary Disks. II. Azimuthal Asymmetries, Different Radial Distributions of Large and Small Dust Grains in PDS~70

J. Hashimoto, T. Tsukagoshi, J. M. Brown +54

The formation scenario of a gapped disk, i.e., transitional disk, and its asymmetry is still under debate. Proposed scenarios such as disk-planet interaction, photoevaporation, gra…

astro-ph.SR2014★ 41 cited

Kinematics of the Outflow From The Young Star DG Tau B: Rotation in the vicinities of an optical jet

Luis A. Zapata, Susana Lizano, Luis F. Rodriguez +4

We present CO(2-1) line and 1300 m continuum observations made with the Submillimeter Array (SMA) of the young star DG Tau B. We find, in the continuum observations, emis…

astro-ph.SR2014★ 14 cited

Radial velocity measurements of the pulsating zirconium star: LS IV -14 116

C. Simon Jeffery, Amir Ahmad, Naslim Neelamkodan +1

The helium-rich hot subdwarf LS IV -14 116 shows remarkably high surface abundances of zirconium, yttrium, strontium, and germanium, indicative of strong chemical stratification in…

astro-ph.SR2014★ 14 cited

A Spitzer Space Telescope survey of extreme Asymptotic Giant Branch stars in M32

O. C. Jones, I. McDonald, R. M. Rich +4

We investigate the population of cool, evolved stars in the Local Group dwarf elliptical galaxy M32, using Infrared Array Camera observations from the Spitzer Space Telescope. We c…

astro-ph.SR2014★ 66 cited

Transition from the Infalling Envelope to the Keplerian Disk around L1551 IRS 5

Ti-Lin Chou, Shigehisa Takakuwa, Hsi-Wei Yen +2

We present combined SubMillimeter Array (SMA) + Atacama Submillimeter Telescope Experiment (ASTE) images of the Class I protobinary L1551 IRS 5 in the CS ( = 7--6) line, the sub…

astro-ph.SR2014★ 19 cited

On the diffuse X-ray emission from the Wolf-Rayet Bubble NGC 2359

J. A. Toalá, M. A. Guerrero, Y. -H. Chu +1

A recent XMM-Newton observation (Zhekov 2014) has revealed diffuse X-ray emission inside the nebula NGC 2359 around the Wolf-Rayet star WR 7. Taking advantage of an improved point-…

astro-ph.SR2014★ 35 cited

Surface Geometry of Protoplanetary Disks Inferred From Near-Infrared Imaging Polarimetry

Michihiro Takami, Yasuhiro Hasegawa, Takayuki Muto +58

We present a new method of analysis for determining the surface geometry of five protoplanetary disks observed with near-infrared imaging polarimetry using Subaru-HiCIAO. Using as…

astro-ph.SR2014★ 64 cited

Angular Momentum Exchange by Gravitational Torques and Infall in the Circumbinary Disk of the Protostellar System L1551 NE

Shigehisa Takakuwa, Masao Saito, Kazuya Saigo +4

We report the ALMA observation of the Class I binary protostellar system L1551 NE in the 0.9-mm continuum, C18O (3-2), and 13CO (3-2) lines at a ~1.6 times higher resolution and a…

astro-ph.SR2014★ 143 cited

A VLBI Resolution of the Pleiades Distance Controversy

Carl Melis, Mark J. Reid, Amy J. Mioduszewski +2

Because of its proximity and its youth, the Pleiades open cluster of stars has been extensively studied and serves as a cornerstone for our understanding of the physical properties…

astro-ph.SR2014★ 36 cited

Characterization of Molecular Outflows in The Substellar Domain

Ngoc Phan-Bao, Chin-Fei Lee, Paul T. P. Ho +2

We report here our latest search for molecular outflows from young brown dwarfs and very low-mass stars in nearby star-forming regions. We have observed three sources in Taurus wit…

astro-ph.SR2014★ 78 cited

Modelling the magnetic activity & filtering radial velocity curves of young Suns: the weak-line T Tauri star LkCa 4

J. -F. Donati, E. Hebrard, G. Hussain +18

We report results of a spectropolarimetric and photometric monitoring of the weak-line T Tauri star LkCa4 within the MaTYSSE programme, involving ESPaDOnS at the Canada-France-Hawa…

astro-ph.SR2014★ 54 cited

On the Role of Pseudodisk Warping and Reconnection in Protostellar Disk Formation in Turbulent Magnetized Cores

Zhi-Yun Li, Ruben Krasnopolsky, Hsien Shang +1

The formation of rotationally supported protostellar disks is suppressed in ideal MHD in non-turbulent cores with aligned magnetic field and rotation axis. A promising way to resol…

astro-ph.SR2014

Spitzer SAGE-Spec: Near Infrared Spectroscopy, Dust Shells, and Cool Envelopes in Extreme Large Magellanic Cloud AGB Stars

R. D. Blum, S. Srinivasan, F. Kemper +2

K-band spectra are presented for a sample of 39 Spitzer IRS SAGE-Spec sources in the Large Magellanic Cloud. The spectra exhibit characteristics in very good agreement with their p…

astro-ph.SR2014★ 10 cited

Early-stage star forming cloud cores in GLIMPSE Extended Green Objects (EGOs) as traced by organic species

Jixing Ge, Jinhua He, Xi Chen +1

In order to investigate the physical and chemical properties of massive star forming cores in early stages, we analyse the excitation and abundance of four organic species, CH3OH,…

astro-ph.SR2014★ 4 cited

CO J = 2 - 1 Emission from Evolved Stars in the Galactic Bulge

Benjamin A. Sargent, N. A. Patel, M. Meixner +3

We observe a sample of 8 evolved stars in the Galactic Bulge in the CO J = 2 - 1 line using the Submillimeter Array (SMA) with angular resolution of 1 - 4 arcseconds. These stars h…

astro-ph.SR2014★ 38 cited

Search for surviving companions in type Ia supernova remnants

Kuo-Chuan Pan, Paul M. Ricker, Ronald E. Taam

The nature of the progenitor systems of type~Ia supernovae is still unclear. One way to distinguish between the single-degenerate scenario and double-degenerate scenario for their…

astro-ph.SR2014★ 120 cited

ALMA Observations of Infalling Flows toward the Keplerian Disk around the Class I Protostar L1489 IRS

Hsi-Wei Yen, Shigehisa Takakuwa, Nagayoshi Ohashi +8

We have conducted ALMA observations in the 1.3 mm continuum and 12CO (2-1), C18O (2-1) and SO (5_6-4_5) lines toward L1489 IRS, a Class I protostar surrounded by a Keplerian disk a…

astro-ph.SR2014★ 107 cited

Carbon-rich dust past the asymptotic giant branch: aliphatics, aromatics, and fullerenes in the Magellanic Clouds

G. C. Sloan, E. Lagadec, A. A. Zijlstra +10

Infrared spectra of carbon-rich objects which have evolved off the asymptotic giant branch reveal a range of dust properties, including fullerenes, polycyclic aromatic hydrocarbons…