output
19932026
Showing 2010 · astro-ph.GAShow all

19 papers · 2 filters

astro-ph.GA2010★ 70 cited

The Dawning of the Stream of Aquarius in RAVE

Mary E. K. Williams, Matthias Steinmetz, Sanjib Sharma +22

We identify a new, nearby (0.5 < d < 10 kpc) stream in data from the RAdial Velocity Experiment (RAVE). As the majority of stars in the stream lie in the constellation of Aquarius…

astro-ph.GA2010★ 106 cited

Detection of a radial velocity gradient in the extended local disc with RAVE

A. Siebert, B. Famaey, I. Minchev +22

Using a sample of 213,713 stars from the Radial Velocity Experiment (RAVE) survey, limited to a distance of 2 kpc from the Sun and to |z|<1 kpc, we report the detection of a veloci…

astro-ph.GA2010★ 20 cited

Towards a new full-sky list of radial velocity standard stars

F. Crifo, G. Jasniewicz, C. Soubiran +4

The calibration of the Radial Velocity Spectrometer (RVS) onboard the ESA Gaia satellite (to be launched in 2012) requires a list of standard stars with a radial velocity (RV) know…

astro-ph.GA2010★ 143 cited

Structure in phase space associated with spiral and bar density waves in an N-body galactic disk

Alice C. Quillen, Jamie Dougherty, Micaela B. Bagley +2

An N-body hybrid simulation, integrating both massive and tracer particles, of a Galactic disk is used to study the stellar phase space distribution or velocity distributions in di…

astro-ph.GA2010★ 2 cited

Radial Mixing due to Spiral-Bar Resonance Overlap: Implications to the Milky Way

I. Minchev, B. Famaey

We have recently identified a previously unknown radial migration mechanism resulting from the overlap of spiral and bar resonances in galactic discs (Minchev & Famaey 2010, Minche…

astro-ph.GA2010★ 56 cited

Testing formation mechanisms of the Milky Way's thick disc with RAVE

Michelle Wilson, Amina Helmi, H. L. Morrison +21

We study the eccentricity distribution of a thick disc sample of stars observed in the Radial Velocity Experiment (RAVE) and compare it to that expected in four simulations of thic…

astro-ph.GA2010★ 29 cited

Rapid Intrinsic Variability of Sgr A* at Radio Wavelengths

F. Yusef-Zadeh, M. Wardle, J. Miller-Jones +3

Sgr A* exhibits flares in radio, millimeter and submm wavelengths with durations of hour. Using structure function, power spectrum and autocorrelation function analysis, w…

astro-ph.GA2010★ 131 cited

The two states of Sgr A* in the near-infrared: bright episodic flares on top of low-level continuous variability

K. Dodds-Eden, S. Gillessen, T. K. Fritz +11

In this paper we examine properties of the variable source Sgr A* in the near-infrared (NIR) using a very extensive Ks-band data set from NACO/VLT observations taken 2004 to 2009.…

astro-ph.GA2010★ 39 cited

The Northern wraps of the Sagittarius Stream as traced by Red Clump stars: distances, intrinsic widths and stellar densities

M. Correnti, M. Bellazzini, R. A. Ibata +2

We trace the tidal Stream of the Sagittarius dwarf spheroidal galaxy (Sgr dSph) using Red Clump stars from the catalog of the Sloan Digital Sky Survey - Data Release 6, in the rang…

astro-ph.GA2010★ 137 cited

The Herschel first look at protostars in the Aquila Rift

S. Bontemps, Ph. Andre, V. Konyves +40

As part of the science demonstration phase of the Herschel mission of the Gould Belt Key Program, the Aquila Rift molecular complex has been observed. The complete ~ 3.3deg x 3.3de…

astro-ph.GA2010★ 34 cited

Herschel photometric observations of the low metallicity dwarf galaxy NGC 1705

B. O'Halloran, M. Galametz, S. C. Madden +57

We present Herschel SPIRE and PACS photometeric observations of the low metallicity (Z ~ 0.35 solar) nearby dwarf galaxy, NGC 1705, in six wavelength bands as part of the Dwarf Gal…

astro-ph.GA2010★ 17 cited

The central region of spiral galaxies as seen by Herschel. M81, M99 and M100

M. Sauvage, N. Sacchi, G. J. Bendo +57

With appropriate spatial resolution, images of spiral galaxies in thermal infrared (~10 micron and beyond) often reveal a bright central component, distinct from the stellar bulge,…

astro-ph.GA2010★ 101 cited

Time Dependent Models of Flares from Sagittarius A*

Katie Dodds-Eden, Prateek Sharma, Eliot Quataert +4

The emission from Sgr A*, the supermassive black hole in the Galactic Center, shows order of magnitude variability ("flares") a few times a day that is particularly prominent in th…

astro-ph.GA2010★ 32 cited

X-ray and multiwavelength view of NGC 4278. A LINER-Seyfert connection?

G. Younes, D. Porquet, B. Sabra +3

(Abridged) Based on UV to X-ray and radio to UV flux ratios, some argue that low ionization emission line regions (LINERs) and low luminosity AGN (LLAGN) are a scaled-down version…

astro-ph.GA2010★ 104 cited

Halo globular clusters observed with AAOmega: dark matter content, metallicity and tidal heating

Richard R. Lane, László L. Kiss, Geraint F. Lewis +6

Globular clusters have proven to be essential to our understanding of many important astrophysical phenomena. Here we analyse spectroscopic observations of ten Halo globular cluste…

astro-ph.GA2010

Multi-Wavelength Study of Sgr A*: The Short Time Scale Variability

F. Yusef-Zadeh, J. Miller-Jones, D. Roberts +5

To understand the correlation and the radiation mechanism of flare emission in different wavelength bands, we have coordinated a number of telescopes to observe SgrA* simultaneousl…

astro-ph.GA2010★ 69 cited

Distance determination for RAVE stars using stellar models

M. A. Breddels, M. C. Smith, A. Helmi +21

(Abridged) Aims:We develop a method for deriving distances from spectroscopic data and obtaining full 6D phase-space coordinates for the RAVE survey's second data release. Methods:…

astro-ph.GA2010

Flares from Sgr A* and their emission mechanism

K. Dodds-Eden, D. Porquet, G. Trap +12

We summarize recent observations and modeling of the brightest Sgr A* flare to be observed simultaneously in (near)-infrared and X-rays to date. Trying to explain the spectral char…

astro-ph.GA2010★ 16 cited

AAOmega Observations of 47 Tucanae: Evidence for a Past Merger?

Richard R. Lane, Brendon J. Brewer, László L. Kiss +6

The globular cluster 47 Tucanae is well studied but it has many characteristics that are unexplained, including a significant rise in the velocity dispersion profile at large radii…