output
19962026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations

Showing 2012 · astro-ph.GAShow all

35 papers · 2 filters

astro-ph.GA2012★ 114 cited

Unveiling a network of parallel filaments in the Infrared Dark Cloud G14.225-0.506

Gemma Busquet, Qizhou Zhang, Aina Palau +10

We present the results of combined NH3(1,1) and (2,2) line emission observed with the Very Large Array and the Effelsberg 100m telescope of the Infrared Dark Cloud G14.225-0.506. T…

astro-ph.GA2012★ 2 cited

Stellar dust production and composition in the Magellanic Clouds

F. Kemper

The dust reservoir in the interstellar medium of a galaxy is constantly being replenished by dust formed in the stellar winds of evolved stars. Due to their vicinity, nearby irregu…

astro-ph.GA2012★ 6 cited

Effects of H2 coating of grains on depletion of molecular species

Oscar Morata, Tatsuhiko I. Hasegawa

Physical conditions in dense and cold regions of interstellar clouds favour the formation of ice mantles on the surfaces of interstellar grains. It is predicted that most of the ga…

astro-ph.GA2012★ 26 cited

Dust continuum and Polarization from Envelope to Cores in Star Formation: A Case Study in the W51 North region

Ya-Wen Tang, Paul T. P. Ho, Patrick M. Koch +2

We present the first high-angular resolution (up to 0.7", ~5000 AU) polarization and thermal dust continuum images toward the massive star-forming region W51 North. The observation…

astro-ph.GA2012★ 81 cited

Hierarchical Fragmentation of the Orion Molecular Filaments

Satoko Takahashi, Paul T. P. Ho, Paula S. Teixeira +2

We present a high angular resolution map of 850 um continuum emission of the Orion Molecular Cloud-3 (OMC 3) obtained with the Submillimeter Array (SMA); the map is a mosaic of 85…

astro-ph.GA2012★ 82 cited

Chemistry in Disks VIII: the CS molecule as an analytic tracer of turbulence in disks

S. Guilloteau, A. Dutrey, V. Wakelam +5

Turbulence is thought to be a key driver of the evolution of protoplanetary disks, regulating the mass accretion process, the transport of angular momentum, and the growth of dust…

astro-ph.GA2012★ 242 cited

The Dependence of Quenching upon the Inner Structure of Galaxies at 0.5<z< 0.8 in the DEEP2/AEGIS Survey

Edmond Cheung, S. M. Faber, David C. Koo +25

The shutdown of star formation in galaxies is generally termed `quenching'. Although quenching may occur through a variety of processes, the exact mechanism(s) that is in fact resp…

astro-ph.GA2012★ 103 cited

Early stages of cluster formation: fragmentation of massive dense cores down to ~1000 AU

Aina Palau, Asunción Fuente, Josep M. Girart +11

In order to study the fragmentation of massive dense cores, which constitute the cluster cradles, we observed with the PdBI in the most extended configuration the continuum at 1.3…

astro-ph.GA2012★ 103 cited

Kiloparsec-scale Radio Structures in Narrow-line Seyfert 1 Galaxies

Akihiro Doi, Hiroshi Nagira, Nozomu Kawakatu +3

We report the finding of kiloparsec (kpc)-scale radio structures in three radio-loud narrow-line Seyfert 1 (NLS1) galaxies from the Faint Images of the Radio Sky at Twenty-centimet…

astro-ph.GA2012★ 121 cited

The circumstellar disk of AB Aurigae: evidence for envelope accretion at late stages of star formation?

Ya-Wen Tang, Stephane Guilloteau, Vincent Pietu +3

The circumstellar disk of AB Aurigae has garnered strong attention owing to the apparent existence of spirals at a relatively young stage and also the asymmetric disk traced in the…

astro-ph.GA2012★ 11 cited

Disentangling the circumnuclear environs of Centaurus A: Gaseous Spiral Arms in a Giant Elliptical Galaxy

D. Espada, S. Matsushita, A. B. Peck +3

We report the existence of spiral arms in the recently formed gaseous and dusty disk of the closest giant elliptical, NGC 5128 (Centaurus A), using high resolution 12CO(2-1) observ…

astro-ph.GA2012★ 50 cited

Milky Way Supermassive Black Hole: Dynamical Feeding from the Circumnuclear Environment

Hauyu Baobab Liu, Pei-Ying Hsieh, Paul T. P. Ho +4

The supermassive black hole (SMBH), Sgr A*, at the Galactic Center is surrounded by a molecular circumnuclear disk (CND) lying between 1.5-4 pc radii. The irregular and clumpy stru…

astro-ph.GA2012★ 13 cited

Young starless cores embedded in the magnetically dominated Pipe Nebula. II. Extended dataset

P. Frau, J. M. Girart, M. T. Beltran +8

The Pipe nebula is a massive, nearby, filamentary dark molecular cloud with a low star-formation efficiency threaded by a uniform magnetic field perpendicular to its main axis. It…

astro-ph.GA2012★ 28 cited

Feathering Instability of Spiral Arms. I: Formulation of the Problem

Wing-Kit Lee, Frank H. Shu

In this paper we study the feathering substructures along spiral arms by considering the perturbational gas response to a spiral shock. Feathers are density fluctuations that jut o…

astro-ph.GA2012★ 12 cited

The chemistry of extragalactic carbon stars

Paul M. Woods, Catherine Walsh, Martin A. Cordiner +1

Prompted by the ongoing interest in Spitzer Infrared Spectrometer spectra of carbon stars in the Large Magellanic Cloud, we have investigated the circumstellar chemistry of carbon…

astro-ph.GA2012★ 36 cited

A Multi-Wavelength High Resolution Study of the S255 Star Forming Region. General structure and kinematics

I. Zinchenko, S. -Y. Liu, Y. -N. Su +4

We present observational data for two main components (S255IR and S255N) of the S255 high mass star forming region in continuum and molecular lines obtained at 1.3 mm and 1.1 mm wi…

astro-ph.GA2012★ 67 cited

Winds of change - a molecular outflow in NGC 1377? The anatomy of an extreme FIR-excess galaxy

S. Aalto, S. Muller, K. Sakamoto +3

We use high (0."65 x 0."52,(65x52pc)) resolution SubMillimeter Array (SMA) observations to image the CO and 13CO 2-1 line emission of the extreme FIR-excess galaxy NGC 1377. We fin…

astro-ph.GA2012★ 553 cited

LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) The survey science plan

Licai Deng, Heidi Jo Newberg, Chao Liu +22

We describe the current plans for a spectroscopic survey of millions of stars in the Milky Way galaxy using the Guo Shou Jing Telescope (GSJT, formerly the Large Area Multi-Object…

astro-ph.GA2012★ 31 cited

The selection of LEGUE disk targets for LAMOST's pilot survey

Li Chen, Jinliang Hou, Jincheng Yu +18

We describe the target selection algorithm for the low latitude disk portion of the LAMOST Pilot Survey, which aims to test systems in preparation for the LAMOST spectroscopic surv…

astro-ph.GA2012★ 4 cited

Probing the physical and chemical structure of the CS core in LDN 673. Multitransitional and continuum observations

Oscar Morata, Josep Miquel Girart, Robert Estalella +1

High-angular resolution observations of dense molecular cores show that these cores can be clumpier at smaller scales, and that some of these clumps can also be unbound or transien…

astro-ph.GA2012★ 224 cited

Dust formation history of galaxies: a critical role of metallicity for the dust mass growth by accreting materials in the interstellar medium

Ryosuke S. Asano, Tsutomu T. Takeuchi, Hiroyuki Hirashita +1

This paper investigate what is the main driver of the dust mass growth in the interstellar medium (ISM) by using a chemical evolution model of galaxy with metals (elements heavier…

astro-ph.GA2012★ 40 cited

Impact of grain size distributions on the dust enrichment in high-redshift quasars

Tzu-Ming Kuo, Hiroyuki Hirashita

In high-redshift () quasars, a large amount of dust ($\textstyle\sim 10^{8} \mathrm{M}_{\sun}$) has been observed. In order to explain the large dust content, we focus on a po…

astro-ph.GA2012★ 19 cited

From dusty filaments to massive stars: The case of NGC 7538 S

Raul Naranjo-Romero, Luis A. Zapata, Enrique Vazquez-Semadeni +3

We report on high-sensitivity and high-angular resolution archival Submillimeter Array (SMA) observations of the large (15000 AU) putative circumstellar disk associated with…

astro-ph.GA2012★ 89 cited

A Keplerian Circumbinary Disk around the Protobinary System L1551 NE

Shigehisa Takakuwa, Masao Saito, Jeremy Lim +3

We present SubMillimeter-Array observations of a Keplerian disk around the Class I protobinary system L1551 NE in 335 GHz continuum emission and submillimeter line emission in 13CO…