[PDF] Top 20 VARIABILITY OF THE EMISSION LINE FLUXES AND RATIOS OF HH 1/2
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VARIABILITY OF THE EMISSION LINE FLUXES AND RATIOS OF HH 1/2
... data of HH 1 and 2 obtained in 1978 (by Brugel et ...with the emission line fluxes from calibrated Hubble Space Telescope (HST) images obtained in 1994 ... See full document
9
The Seyfert 2 galaxy NGC 2110: hard X ray emission observed by NuSTAR and variability of the iron K alpha line
... 100024010) and seven years later, starting on 2012 August 31 (OBSID ...from the X-ray Imaging Spectrometer (XIS) and the Hard X-ray Detector ...reprocessed the event files with ... See full document
12
Long-term variability of the optical spectra of NGC4151. II. Evolution of the broad Hα and Hβ emission-line profiles.
... that of the continuum (Paper 1), we infer that the change in the inte- grated Balmer decrement during 1999−2001 is also caused, at least partially, by changes in the continuum ... See full document
20
A COMPARISON OF THE RADIO AND OPTICAL TIME-EVOLUTION OF HH 1 AND 2
... • HH 2 shows a general trend of increasing in- tensities, with condensation H becoming much brighter and condensation A fading ...away. The fact that both the radio and ... See full document
8
The Transverse Velocity Structure of the HH 111 Jet
... Figure 2, we present the [S II] 6731 ˚ A position- velocity diagram (panel a), radial velocities (panel b), as well as the [S II] 6717/6731 and [S II] (6717+6731)/Hα ratios (panels c ... See full document
11
Emission Line Ratios from Variable Velocity Jet Models
... between the line ratios predicted for the knots of our jet mod- els (see also Table 2), the “self-consistent preion- ization”, stationary, plane-parallel shock models ... See full document
12
Fabry-Perot Observations of HH 1/2
... For HH 2 (see ...for the radial velocity barycenter of the line profiles, with a complex interface between the red- and blue- shifted ...regions. The radial ... See full document
12
The Photometric Variability of HH 30
... panels of Figures 3 and 4 show peri- odograms calculated after binning the data into bins of 1/8 of the ...period. The fourth panel in each figure shows the ... See full document
11
Review An overview of the observational and theoretical studies of HH 1 and 2
... modelling HH 1 (Raga 1988; Blondin et al. 1989; V¨ olker et al. 1999) and HH 2 (Stone & Norman 1994) with full (axisymmetric or 3D) jet simulations, more work in this direction ... See full document
13
BAT AGN spectroscopic survey II X ray emission and high ionization optical emission lines
... GS-2010A-Q-54, and GS-2011B- Q80 were used in this publication. We acknowledge the work that the Swift BAT team has done to make this work ...possible. The Kitt Peak National Observatory ... See full document
13
Ly alpha EMITTING GALAXIES AT z=2 1 IN ECDF S: BUILDING BLOCKS OF TYPICAL PRESENT DAY GALAXIES?
... compares the SFRs measured from UV and Lyα. The reduced density of objects at the upper left (SFR(UV) > 10 M yr −1 ) and lower left (SFR(UV) < 2 M yr ... See full document
15
The how and why of the expansion of public higher education in Brazil
... from the 2009 National Household Sample (pnad, 2010), in regards to the relationship between schooling and family income, the North and Northeast regions have the worst rates ... See full document
18
Morphological variability of the nanoplanktonic diatom Thalassiosira laevis from coastal waters of Province of Buenos Aires (Argentina) - Sociedad Argentina de Botánica
... waters of the Province of Buenos Aires (Fig. 1). The sampling stations in the Province of Buenos Aires were: San Clemente del Tuyú (36º 21' 16'' S–56º 42' 54'' W), Santa ... See full document
6
Spectroscopy of the short hard GRB 130603B The host galaxy and environment of a compact object merger â
... gamma-ray emission, into two distinctive types: long, with typi- cal durations of more than 2 s and soft spectra, or short, lasting less than 2 s and with harder spectra ... See full document
17
Monitoring of airborne biological particles in outdoor atmosphere. Part 1: Importance, variability and ratios
... Some of these organisms, or just parts of them, can cause allergies, disorders and diseases in humans and other animals, with important health and economical conse- ...conditions ... See full document
14
New insights and methods for the clustering of emission line galaxies
... shows the 2PCFs of the dark matter, the SAG sample, and the shuffled sample, for di ff erent ...for the 2-halo regime only (log(r/Mpc h −1 ) & 0). ... See full document
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SPECTRAL BEHAVIOR OF THE SYMBIOTIC NOVA HM SGE IN THE ULTRAVIOLET
... variety of emission lines with different ionization states be- cause not all systems have a ...nebula. The absence of emission lines may be due to the high density of ... See full document
7
A Study of the Variability of Water Maser Emission in a Sample of Young Stellar Objects
... (1993) and Lekht & Sorochenko ...spectrum of three maser features; the central com- ponent has a velocity close to that of the molecu- lar cloud, and the lateral ones ... See full document
20
The Use of Line Excitation Mapping to Investigate Planetary Nebula Morphologies
... variety of shapes, although it appears that approximately 85% may be classified as circular, el- liptical, or bipolar (Manchado et ...whims of the formation process, but appear to reflect deeper- ... See full document
16
Gas and dust in a submillimeter galaxy at ⱬ = 4.24 from the herschel atlas
... at the IRAM 30 m telescope on 2010 May 19 using the 117 channel Max-Planck Millimeter Bolometer or MAMBO-2 array to measure the dust continuum flux density at ...mm. The observations ... See full document
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