scholarly journals Unveiling the Central Parsec Region of an Active Galactic Nucleus: The Circinus Nucleus in the Near‐Infrared with the Very Large Telescope

2004 ◽  
Vol 614 (1) ◽  
pp. 135-141 ◽  
Author(s):  
M. Almudena Prieto ◽  
K. Meisenheimer ◽  
Olivier Marco ◽  
Juha Reunanen ◽  
Marcella Contini ◽  
...  
Keyword(s):  
Active Galactic Nucleus ◽  
Near Infrared ◽  
Large Telescope ◽  
Very Large Telescope ◽  
Central Parsec

scholarly journals Unidentified emission features in the R Coronae Borealis star V854 Centauri

2018 ◽  
Vol 610 ◽  
pp. L6 ◽  
Author(s):  
L. C. Oostrum ◽  
B. B. Ochsendorf ◽  
L. Kaper ◽  
A. G. G. M. Tielens
Keyword(s):  
Near Infrared ◽  
Physical Nature ◽  
The Other ◽  
Large Telescope ◽  
Circumstellar Material ◽  
Spatially Resolved ◽  
Broad Emission ◽  
Very Large Telescope ◽  
New Feature ◽  
Molecular Nature

During its 2012 decline, the R Coronae Borealis star (RCB) V854 Cen was spectroscopically monitored with X-shooter on the ESO Very Large Telescope. The obscured optical and near-infrared spectrum exhibits many narrow and several broad emission features, as previously observed. The envelope is spatially resolved along the slit and allows for a detailed study of the circumstellar material. In this Letter, we report on the properties of a number of unidentified visual emission features (UFs), including the detection of a new feature at 8692 Å. These UFs have been observed in the Red Rectangle (RR), but their chemical and physical nature is still a mystery. The previously known UFs behave similarly in the RR and in V854 Cen, but are not detected in six other observed RCBs. Some hydrogen might be required for the formation of their carrier(s). The λ8692 UF is present in all RCBs. Its carrier is likely of a carbonaceous molecular nature, presumably different from that of the other UFs.

scholarly journals The dwarf planet Makemake as seen by X-Shooter

2020 ◽  
Vol 497 (4) ◽  
pp. 5473-5479
Author(s):  
Alvaro Alvarez-Candal ◽  
Ana Carolina Souza-Feliciano ◽  
Walter Martins-Filho ◽  
Noemí Pinilla-Alonso ◽  
José Luis Ortiz
Keyword(s):  
Infrared Spectrum ◽  
Near Infrared ◽  
Resolving Power ◽  
Large Telescope ◽  
Very Large Telescope ◽  
Absorption Features ◽  
Near Infrared Spectrum

ABSTRACT Makemake is one of the brightest known trans-Neptunian objects, as such, it has been widely observed. Nevertheless, its visibility to near-infrared spectrum has not been completely observed in medium-resolving power, aimed at studying in detail the absorption features of CH4 ice. In this paper, we present the spectrum of Makemake observed with X-Shooter at the Very Large Telescope (Chile). We analyse the detected features, measuring their location and depth. Furthermore, we compare Makemake’s spectrum with that of Eris, obtained with the same instrument and similar setup, to conclude that the bands of the CH4 ice in both objects show similar shifts.

scholarly journals Polarimetry of relativistic tidal disruption event Swift J2058+0516

2019 ◽  
Vol 491 (2) ◽  
pp. 1771-1776 ◽  
Author(s):  
K Wiersema ◽  
A B Higgins ◽  
A J Levan ◽  
R A J Eyles ◽  
R L C Starling ◽  
...  
Keyword(s):  
Linear Polarization ◽  
Near Infrared ◽  
Thermal Emission ◽  
Large Telescope ◽  
Relativistic Jets ◽  
Tidal Disruption ◽  
Very Large Telescope ◽  
Wide Range ◽  
Independent Test ◽  
Show Evidence

ABSTRACT A small fraction of candidate tidal disruption events (TDEs) show evidence of powerful relativistic jets, which are particularly pronounced at radio wavelengths, and likely contribute non-thermal emission at a wide range of wavelengths. A non-thermal emission component can be diagnosed using linear polarimetry, even when the total received light is dominated by emission from an accretion disc or disc outflow. In this paper, we present Very Large Telescope (VLT) measurements of the linear polarization of the optical light of jetted TDE Swift J2058+0516. This is the second jetted TDE studied in this manner, after Swift J1644+57. We find evidence of non-zero optical linear polarization, $P_{V}\sim 8{{\, \rm per\, cent}}$, a level very similar to the near-infrared polarimetry of Swift J1644+57. These detections provide an independent test of the emission mechanisms of the multiwavelength emission of jetted TDEs.

Very Large Telescope–ISAAC Near-Infrared Spectroscopy of [ITAL]ISO[/ITAL]-selected Hubble Deep Field South Galaxies

2000 ◽  
Vol 537 (2) ◽  
pp. L85-L89 ◽  
Author(s):  
D. Rigopoulou ◽  
A. Franceschini ◽  
H. Aussel ◽  
R. Genzel ◽  
P. van der Werf ◽  
...  
Keyword(s):  
Infrared Spectroscopy ◽  
Near Infrared Spectroscopy ◽  
Near Infrared ◽  
Large Telescope ◽  
Very Large Telescope ◽  
Hubble Deep Field

scholarly journals Detection and characterization of two VLM binaries: LP 1033-31 and LP 877-72

2020 ◽  
Vol 498 (1) ◽  
pp. 737-749
Author(s):  
Subhajeet Karmakar ◽  
A S Rajpurohit ◽  
F Allard ◽  
D Homeier
Keyword(s):  
Adaptive Optics ◽  
Spectral Type ◽  
Near Infrared ◽  
Binding Energies ◽  
Secondary Component ◽  
Large Telescope ◽  
Very Large Telescope ◽  
Adaptive Optics Imaging ◽  
M Dwarf

ABSTRACT Using the high-resolution near-infrared adaptive optics imaging from the NaCo instrument at the Very Large Telescope, we report the discovery of a new binary companion to the M-dwarf LP 1033-31 and also confirm the binarity of LP 877-72. We have characterized both the stellar systems and estimated the properties of their individual components. We have found that LP 1033-31 AB with the spectral type of M4.5+M4.5 has a projected separation of 6.7 ± 1.3 AU. Whereas with the spectral type of M1+M4, the projected separation of LP 877-72 AB is estimated to be 45.8 ± 0.3 AU. The binary companions of LP 1033-31 AB are found to have similar masses, radii, effective temperatures, and log g with the estimated values of 0.20 ± 0.04 $\rm {M}_{\odot }$, 0.22 ± 0.03 $\rm {R}_{\odot }$, and 3200 K, 5.06 ± 0.04. However, the primary of LP 877-72 AB is found to be twice as massive as the secondary with the derived mass of 0.520 ± 0.006 $\rm {M}_{\odot }$. The radius and log g for the primary of LP 877-72 AB are found to be 1.8 and 0.95 times that of the secondary component with the estimated values of 0.492 ± 0.011 $\rm {R}_{\odot }$ and 4.768 ± 0.005, respectively. With an effective temperature of 3750 ± 15 K, the primary of LP 877-72 AB is also estimated to be ∼400 K hotter than the secondary component. We have also estimated the orbital period of LP 1033-31 and LP 877-72 to be ∼28 and ∼349 yr, respectively. The binding energies for both systems are found to be >1043 erg, which signifies that both systems are stable.

Sign in / Sign up

Export Citation Format

Share Document