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相关论文: The detection of [Ne v] emission in five blue comp…

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The discovery of the high-ionization [Ne V] 3426A emission line in the spectrum of the blue compact dwarf (BCD) galaxy Tol 1214-277 is reported. The detection of this line implies the presence of intense ionizing X-ray emission with a…

天体物理学 · 物理学 2009-11-10 Y. I. Izotov , K. G. Noeske , N. G. Guseva , P. Papaderos , T. X. Thuan , K. J. Fricke

We report the discovery of [NeV]3426 emission, in addition to HeII4686 emission, in six compact star-forming galaxies. These observations considerably increase the sample of eight such galaxies discovered earlier by our group. For four of…

星系天体物理 · 物理学 2021-10-19 Y. I. Izotov , T. X. Thuan , N. G. Guseva

Primordial stars are expected to be very massive and hot, producing copious amounts of hard ionizing radiation. The best place to study hard ionizing radiation in the local universe is in very metal-deficient Blue Compact Dwarf (BCD)…

天体物理学 · 物理学 2018-05-30 T. X. Thuan , Y. I. Izotov

We analyze a sample of 25 [Ne V] $\lambda$3426 emission-line galaxies at $1.4<z<2.3$ using Hubble Space Telescope/Wide Field Camera 3 G102 and G141 grism observations from the CANDELS Lyman-$\alpha$ Emission at Reionization (CLEAR) survey.…

The results of deep long-slit spectroscopy of the extremely low-metallicity blue compact dwarf (BCD) galaxy SBS 0335-052 are presented. Down to intensity levels of 10^{-3 ... -4} of Hbeta, unprecedented for spectroscopy of extra-galactic…

天体物理学 · 物理学 2009-11-07 Y. I. Izotov , F. H. Chaffee , D. Schaerer

We present near-infrared (NIR) spectroscopic observations in the wavelength range 0.90-2.40mum of eighteen low-metallicity blue compact dwarf (BCD) galaxies and six HII regions in spiral and interacting galaxies. Hydrogen and helium…

星系天体物理 · 物理学 2023-05-03 Y. I. Izotov , T. X. Thuan

We investigate the high-ionization, narrow [Ne v] $\lambda$3427 emission line in a sample of over 340 ultrahard X-ray (14-195 keV) selected Active Galactic Nuclei (AGN) drawn from the BASS project. The analysis includes measurements in…

We present an analysis of the mid-infrared emission lines for a sample of 12 low metallicity Blue Compact Dwarf (BCD) galaxies based on high resolution observations obtained with Infrared Spectrograph on board the {\rm Spitzer} Space…

宇宙学与河外天体物理 · 物理学 2015-05-14 Lei Hao , Yanling Wu , V. Charmandaris , H. W. W. Spoon , J. Bernard-Salas , D. Devost , V. Lebouteiller , J. R. Houck

We present two-dimensional spectroscopy of the extremely metal-deficient blue compact dwarf (BCD) galaxy SBS 0335-052E aiming to studyphysical conditions, element abundances and kinematical properties of the ionised gas in this galaxy.…

天体物理学 · 物理学 2018-05-30 Y. Izotov , D. Schaerer , A. Blecha , F. Royer , N. Guseva , P. North

We present 3.5m Apache Point Observatory second-epoch spectra of four low-metallicity emission-line dwarf galaxies discovered serendipitously in the Data Release 5 of the Sloan Digital Sky Survey (SDSS) to have extraordinary large broad…

天体物理学 · 物理学 2018-05-30 Y. I. Izotov , T. X. Thuan

We present spectra of a large sample of low-metallicity blue compact dwarf galaxies which exhibit broad components in their strong emission lines, mainly in Hbeta, [O III]4959, 5007 and Halpha. Twenty-three spectra have been obtained with…

天体物理学 · 物理学 2018-05-30 Y. I. Izotov , T. X. Thuan , N. G. Guseva

We report the discovery of blue shifted (delta(V) > 200 km/s) mid-infrared [NeIII] and/or [NeV] emission in 25 out of 82 ULIRGs (30% of our sample). The incidence of blue shifted [NeV] emission is even higher (59%) among the sources with a…

宇宙学与河外天体物理 · 物理学 2015-05-13 H. W. W. Spoon , J. Holt

We present HST/ACS images and color-magnitude diagrams for 25 nearby galaxies with radial velocities V_LG < 500 km/s. Distances are determined based on the luminosities of stars at the tip of the red giant branch that range from 2 Mpc to 12…

We present near-infrared (NIR) spectroscopic observations of five blue compact dwarf (BCD) galaxies, II Zw 40, Mrk 71, Mrk 930, Mrk 996 and SBS 0335-052E. The NIR spectra which cover the 0.90 micron - 2.40 micron wavelength range, show…

宇宙学与河外天体物理 · 物理学 2018-05-29 Y. I. Izotov , T. X. Thuan

We report the detection of [Ne II] emission at 12.81 micron in four out of the six optically thick dust disks observed as part of the FEPS Spitzer Legacy program. In addition, we detect a H I(7-6) emission line at 12.37 micron from the…

We use the narrow [Ne v] $\lambda$3427 emission line detected in the recently published JWST spectra of two galaxies, at z = 6.9 and 5.6, to study the key properties of the active galactic nuclei (AGN) and the supermassive black holes…

We present a detailed analysis of the most luminous and obscured Active Galactic Nuclei (AGNs) detected in the ultra-hard X-ray band (14-195 keV) by Swift/BAT. Our sample comprises 21 X-ray luminous (log $L_X/{\rm erg\,s^{-1}}>44.6$, 2-10…

We present the results of high spatial resolution HI observations of five intrinsically compact dwarf galaxies which are currently experiencing a strong burst of star formation. The HI maps indicate that these systems have a complex and…

天体物理学 · 物理学 2009-10-30 L. van Zee , E. D. Skillman , J. J. Salzer

Detecting Active Galactic Nuclei (AGN) in galaxies dominated by powerful nuclear star formation and extinction effects poses a unique challenge. Due to the longer wavelength emission and the ionization potential of Ne^3+, infrared [Ne V]…

天体物理学 · 物理学 2009-11-13 N. P. Abel , S. Satyapal

Aiming to find new extremely metal-deficient star-forming galaxies we extracted from the Two-Degree Field Galaxy Redshift Survey (2dFGRS) 100K Data Release 14 emission-line galaxies with relatively strong [OIII] 4363 emission. Spectroscopic…

天体物理学 · 物理学 2009-11-11 P. Papaderos , N. G. Guseva , Y. I. Izotov , K. G. Noeske , T. X. Thuan , K. J. Fricke
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