Figure 8 Global H i emission profile of NGC 6907 and 6908

Slides:

Advertisements

Similar presentations

HI Stacking: Past, Present and Future HI Pathfinder Workshop Perth, February 2-4, 2011 Philip Lah.

Advertisements

Search for new Luminous Blue Variables (1) (Kniazev: RSA_OTH RSA_OTH-014) Vasilii Gvaramadze (SAI MSU) & Alexei Kniazev.

© 2007 Thomson Brooks/Cole, a part of The Thomson Corporation. FIGURES FOR CHAPTER 8 ESTIMATION OF PARAMETERS AND FITTING OF PROBABILITY DISTRIBUTIONS.

Simulations for the nearby Seyfert 2 galaxy NGC 4945 Lien-Hsuan Lin 1,2, Chi Yuan 2, C.C. D. Yen 3, and S. Muller 2 1 Department of Physics, National Taiwan.

Date of download: 7/7/2016 Copyright © ASME. All rights reserved. From: Energy Conservative Dissipative Particle Dynamics Simulation of Natural Convection.

Figure 1. HATLAS J (z = , marked with vertical line)

From: Ion chemistry in the coma of comet 67P near perihelion

Figure 2. A comparison between the modern PMS spectral type-to-effective temperature conversion scales of Pecaut & Mamajek (2013, solid red line, labelled.

Figure 1. Left – a small region of a typical polarized spectrum acquired with the ESPaDOnS instrument during the MiMeS project. This figure illustrates.

From: Discovery of carbon-rich Miras in the Galactic bulge

Table 1. Details of the HST WFPC2 imaging and WHT ISIS spectroscopy presented in this paper. The F656N filter has central wavelength λ6560 Å and a FWHM.

From: The VISTA Deep Extragalactic Observations (VIDEO) survey★

From: Numerical aspects of giant impact simulations

From: The evolution of star formation activity in galaxy groups

Figure 1. Three light curves of IRAS 13224–3809 in 600-s bins

Figure 1. (a) A set-up used for the measurements showing the head phantom and the ion chamber located in the central hole. The cylindrical phantom has.

Figure 2. The residuals to a phenomenological continuum model, revealing strong features at the iron L, iron K, and Compton hump bands. The data are from.

Figure 3. Inclination instability in the outer Solar system

Date of download: 11/12/2017 Copyright © ASME. All rights reserved.

Date of download: 11/16/2017 Copyright © ASME. All rights reserved.

Journal of Vision. 2008;8(11):18. doi: / Figure Legend:

Fig. 2. Semi-major axis vs. eccentricity (left) and semi-major axis vs

Figure Legend: From: The resolution of facial expressions of emotion

Figure 1. The redshift distribution of a GRB sample population.

Genomic Patterns of Homozygosity in Worldwide Human Populations

From: Refugee Migration and Electoral Outcomes

+ = Climate Responses to Biomass Burning Aerosols over South Africa

Diffusion-weighted magnetic resonance imaging in preoperative assessment of non– small cell lung cancer Hiroaki Nomori, MD, Yue Cong, MD, Masaru Abe,

Figure 1. Position vectors of the components – Sun, Earth, Moon and particle (P) – of the studied four-body problem in the barycentric ecliptic coordinate.

Efficient Receptive Field Tiling in Primate V1

Comparison of Microsatellites Versus Single-Nucleotide Polymorphisms in a Genome Linkage Screen for Prostate Cancer–Susceptibility Loci Daniel J. Schaid,

Jason W. Christie, MD, Thomas D. Conlee, MD, Timothy E

Volume 98, Issue 11, Pages (June 2010)

Membrane Permeability of Hydrocarbon-Cross-Linked Peptides

Prescribed forcings. Prescribed forcings. (Top) Volcanic forcing is indicated as global visible optical depth. (Middle) Solar forcing is obtained by scaling.

Surface Brightness Profile - NGC 3379 (giant elliptical)

Volume 55, Issue 3, Pages (August 2007)

Estimated probability of successful quitting (quit attempt of longer than 1 year) by quit attempt number in the Ontario Tobacco Survey. Estimated probability.

A Switching Observer for Human Perceptual Estimation

Increasing Sensitivity of Ca2+ Spark Detection in Noisy Images by Application of a Matched-Filter Object Detection Algorithm Cherrie H.T. Kong, Christian.

Volume 66, Issue 4, Pages (May 2010)

Vassili Ivanov, Min Li, Kiyoshi Mizuuchi Biophysical Journal

Raft Formation in Lipid Bilayers Coupled to Curvature

A Switching Observer for Human Perceptual Estimation

Volume 100, Issue 5, Pages (March 2011)

Volume 114, Issue 5, Pages (March 2018)

Volume 101, Issue 4, Pages (August 2011)

Volume 103, Issue 10, Pages (November 2012)

The cell cycle influences circadian phase progression Circadian intervals with divisions (p1,d1,p2) last 21.95 ± 3.8 h (n = 1,926) and are significantly.

Analyzing Graphs of Functions

Volume 97, Issue 4, Pages (August 2009)

FIGURE 1 Flow chart showing the number of individuals at each stage of the experiment. Among the 61 dyads who ... FIGURE 1 Flow chart showing the number.

“Violent Relaxation” of Star Cluster

Newsome S.J. , Daniel R.M. , Carr S.B. , Bilton D. , Keogh R.H.

Volume 24, Issue 8, Pages e6 (August 2018)

When Correlation Implies Causation in Multisensory Integration

Measuring Actin Flow in 3D Cell Protrusions

Figure 1. Observed mean (SD) micafungin plasma concentrations.

Cytoskeletal Control of Antigen-Dependent T Cell Activation

Molecular Dynamics Simulations of Hydrophilic Pores in Lipid Bilayers

Fig. 1 Bands and hybridization in graphene-encapsulated WSe2 measured by μ-ARPES. Bands and hybridization in graphene-encapsulated WSe2 measured by μ-ARPES.

Volume 66, Issue 4, Pages (May 2010)

Reliability of Assessment of Protein Structure Prediction Methods

Kevin McHale, Andrew J. Berglund, Hideo Mabuchi Biophysical Journal

A simple rule of thumb for elegant prehension

Relationships between species richness and temperature or latitude

Absolute survival probability (per cent who have not quit successfully) of reported quit attempts of longer than 1 year during the first 18 months of observation.

Efficient Receptive Field Tiling in Primate V1

Fig. 5 Superpositions of OAM.

George D. Dickinson, Ian Parker Biophysical Journal

Presentation transcript:

Figure 8 Global H i emission profile of NGC 6907 and 6908 Figure 8 Global H i emission profile of NGC 6907 and 6908. The bottom dotted lines limit the noise level while the top dotted line indicates the maximum emission h. Inside the distribution, two horizontal dashed lines are used to mark the H i line-widths estimated at 20 per cent (w<sub>20</sub>) and at 50 per cent (w<sub>50</sub>) of the peak intensities; v is the central weighted mean velocity distribution. From: H i aperture synthesis and optical observations of the pair of galaxies NGC 6907 and 6908 Mon Not R Astron Soc. 2008;386(2):963-972. doi:10.1111/j.1365-2966.2008.13079.x Mon Not R Astron Soc | © 2008 The Authors. Journal compilation © 2008 RAS 1