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相关论文: Extended CIII]lambda1909 emission in Q0957+561

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We extend the gr-band time coverage of the gravitationally lensed double quasar Q0957+561. New gr light curves permit us to detect significant intrinsic fluctuations, to determine new time delays, and thus to gain perspective on the…

天体物理学 · 物理学 2009-11-13 V. N. Shalyapin , L. J. Goicoechea , E. Koptelova , A. Ullan , R. Gil-Merino

We present Plateau de Bure Interferometer observations of far infra-red emission lines in BRI 0952-0115, a lensed quasar at z=4.4 powered by a super-massive black hole (M_BH=2x10^9 M_sun). In this source, the resolved map of the [CII]…

宇宙学与河外天体物理 · 物理学 2012-11-06 Simona Gallerani

PSR B1259-63 is a middle-aged radio pulsar (P=48 ms, tau=330 kyr, Edot=8.3*10^{35} erg/s) in an eccentric binary (P_orb =3.4 yr, e=0.87) with a high-mass Be companion, SS 2883. We observed the binary near apastron with the Chandra ACIS…

高能天体物理现象 · 物理学 2015-05-20 George G. Pavlov , Chulhoon Chang , Oleg Kargaltsev

We present the first results from a program searching for extended Ly$\alpha$ halos around high redshift ($ z \gtrsim 6.5$) quasars using the red channel of the Keck Cosmic Web Imager (KCWI). Our observations reveal a Ly$\alpha$ halo…

We present high spatial resolution maps, obtained with the Plateau de Bure Interferometer, of the blue lobe of the L1157 outflow. We observed four lines at 3 mm, namely CH3OH (2_K-1_K), HC3N (11-10), HCN (1-0) and OCS (7-6). Moreover, the…

LS 5039 is a high-mass binary with a period of 4 days, containing a compact object and an O star, one of the few high-mass binaries detected in gamma-rays. Our Chandra ACIS observation of LS 5039 provided a high-significance (~10sigma)…

高能天体物理现象 · 物理学 2015-05-27 Martin Durant , Oleg Kargaltsev , George G. Pavlov , Chulhoon Chang , Gordon P. Garmire

The quadruply lensed quasar HE0435-1223 shows a clear microlensing effect that affects differently the blue and red wings of the H$\alpha$ line profile in its image D. To interpret these observations, and constrain the broad emission line…

星系天体物理 · 物理学 2019-09-04 D. Hutsemékers , L. Braibant , D. Sluse , R. Goosmann

SMM J04542-0301 is an extended (~1 arcmin) sub-mm source located near the core of the cluster MS0451.6-0305. It has been suggested that part of its emission arises from the interaction between a LBG and two EROs at z~2.9 that are…

宇宙学与河外天体物理 · 物理学 2015-05-14 A. Berciano Alba , L. V. E. Koopmans , M. A. Garrett , O. Wucknitz , M. Limousin

We have carried out a systematic analysis of the gamma-ray bursts' (GRBs) light curves detected in the SPI-ACS experiment onboard the INTEGRAL observatory aimed to search extended emission. The emission occasionally recorded after the…

高能天体物理现象 · 物理学 2023-09-07 G. Yu. Mozgunov , P. Yu. Minaev , A. S. Pozanenko

We present an analysis of infrared/optical/ultraviolet spectra of the two images of the first gravitationally lensed quasar Q0957+561A, B. The Hubble Space Telescope observations of Q0957+561A and Q0957+561B are separated in time by the…

天体物理学 · 物理学 2009-11-10 Luis J. Goicoechea , Rodrigo Gil-Merino , Aurora Ullan

We present a molecular line study towards 31 extended green object (EGO) clumps in the southern sky using data from MALT90 (Millimetre Astronomy Legacy Team 90 GHz). According to previous multiwavelength observations, we divide our sample…

星系天体物理 · 物理学 2017-02-14 Naiping Yu , Jun-Jie Wang

ALMA observations have revealed that [CII] 158$\mu$m line emission in high-z galaxies is ~2-3$\times$ more extended than the UV continuum emission. Here we explore whether surface brightness dimming (SBD) of the [CII] line is responsible…

Himiko is one of the most luminous Ly{\alpha} emitters at z = 6.595. It has three star forming clumps detected in the rest-frame UV, with a total SFR = 20 M$_\odot$/yr. We report the ALMA detection of the [CII]158$\mu$m line emission in…

星系天体物理 · 物理学 2018-02-21 S. Carniani , R. Maiolino , R. Smit , R. Amorín

This paper presents observations of an extended Lyman-alpha emission nebula surrounding the galaxy responsible for the Damped Lyman-alpha Absorption (DLA) line in the spectrum of the quasar Q2233+131. With the Potsdam Multi Aperture…

天体物理学 · 物理学 2007-05-23 L. Christensen , S. F. Sanchez , K. Jahnke , T. Becker , L. Wisotzki , A. Kelz , L. C. Popovic , M. M. Roth

Observations with the 6-m telescope of the Special Astrophysical Observatory obtained with the MPFS integral-field spectrograph and a longslit spectrograph with the SCORPIO focal reducer are used to analyze the emission spectrum of the…

天体物理学 · 物理学 2008-11-26 V. P. Arkhipova , T. A. Lozinskaya , A. V. Moiseev , O. V. Egorov

We present a 50 ks observation of the gamma-ray binary LSI+61303 carried out with the ACIS-I array aboard the Chandra X-ray Observatory. This is the highest resolution X-ray observation of the source conducted so far. Possible evidence of…

天体物理学 · 物理学 2009-11-13 J. M. Paredes , M. Ribo , V. Bosch-Ramon , J. R. West , Y. M. Butt , D. F. Torres , J. Marti

Deep U-band FOC images of the nuclear region of NGC6251 have revealed a region of extended emission which is most probably radiation scattered from a continuum source in the nucleus. This radiation lies interior to a dust ring, is nearly…

天体物理学 · 物理学 2009-10-30 P. Crane , J. Vernet

SDSS J0924+0219 is the most glaring example of a gravitational lens with anomalous flux ratios: optical broad-band photometry shows image D to be a factor of 12 fainter than expected for smooth lens potentials. We report spectroscopy…

天体物理学 · 物理学 2009-11-13 Charles R. Keeton , Scott Burles , Paul L. Schechter , Joachim Wambsganss

We report long-slit spectroscopic observations of the quasar SDSS J082303.22+052907.6 ($z_{\rm CIV}$$\sim$3.1875), whose Broad Line Region (BLR) is partly eclipsed by a strong damped Lyman-$\alpha$ (DLA; log$N$(HI)=21.7) cloud. This allows…

Models that seek to unify BL Lacs and low-power radio galaxies predict that the two types of object should show similar isotropically emitted X-ray emission. Testing this is usually limited by difficulties in separating strong X-ray…

天体物理学 · 物理学 2009-10-31 M. J. Hardcastle , D. M. Worrall , M. Birkinshaw