scholarly journals Resolving the dusty circumstellar environment of the A[e] supergiant HD 62623 with the VLTI/MIDI

2010 ◽  
Vol 6 (S272) ◽  
pp. 406-407
Author(s):  
Antony Meilland ◽  
Sameer Kanaan ◽  
Marcelo Borges Fernandes ◽  
Olivier Chesneau ◽  
Florentin Millour ◽  
...  

AbstractHD 62623 is one of the very few A-type supergiants showing the B[e] phenomenon. We studied the geometry of its circumstellar envelope in the mid-infrared using the VLTI/MIDI instrument. Using the radiative transfer code MC3D, we managed to model it as a dusty disk with an inner radius of 3.85 AU, an inclination angle of 60°, and a mass of 2 × 10−7M⊙. It is the first time that the dusty disk inner rim of a supergiant star exhibiting the B[e] phenomenon is significantly constrained. The inner gaseous envelope likely contributes up to 20% to the total N band flux and acts like a reprocessing disk. Finally, the hypothesis of a stellar wind deceleration by the companion gravitational effect remains the most probable case since the bi-stability mechanism is not efficient for this star.

2014 ◽  
Vol 9 (S307) ◽  
pp. 389-390
Author(s):  
Coralie Neiner ◽  

AbstractUVMag is a medium-size space telescope equipped with a high-resolution spectropolarimetrer working in the UV and visible domains. It will be proposed to ESA for a future M mission. It will allow scientists to study all types of stars as well as e.g. exoplanets and the interstellar medium. It will be particularly useful for massive stars, since their spectral energy distribution peaks in the UV. UVMag will allow us to study massive stars and their circumstellar environment (in particular the stellar wind) spectroscopically in great details. Moreover, with UVMag's polarimetric capabilities we will be able, for the first time, to measure the magnetic field of massive stars simultaneously at the stellar surface and in the wind lines, i.e. to completely map their magnetosphere.


2019 ◽  
Vol 624 ◽  
pp. A145 ◽  
Author(s):  
J. Souchay ◽  
C. Gattano ◽  
A. H. Andrei ◽  
D. Souami ◽  
B. Coelho ◽  
...  

Context. In addition to their great astrophysical interest, quasars represent quasi-ideal reference objects in the celestial sphere with, a priori, a lack of significant proper motion. Since the fourth release of the Large Quasar Astrometric Catalogue (LQAC-4), a large number of quasars have been discovered, in particular those coming from the DR14Q release of the SDSS. With the advent of the Gaia Data Release 2 (DR2), it is now also possible to fold in extremely accurate quasar positions. Aims. Following the same procedure as in the previous releases of the LQAC, our aim is to compile the large majority of the recorded quasars, with their best estimated coordinates and substantial information about their physical properties such as the redshift, multi-bands apparent, and absolute magnitudes. Emphasis is given to the results of the cross-matches with the Gaia DR2 catalogue, which considerably increases the positional accuracy. Methods. New quasars from the SDSS DR14Q release were cross-matched with the precedent LQAC-4 compilation with a 1″ search radius, which leads to 149 084 objects not present in the previous LQAC-4 release. Another cross-match was done with the Gaia DR2 catalogue, which enables us to considerably improve the positioning of these objects. For the first time, parallaxes and proper motions from the DR2, when available, are added to our compilation. Furthermore, a cross-identification of the LQAC-5 with the AllWISE survey gives additional mid-infrared information for an important percentage of objects. Results. Our final catalogue, namely the LQAC-5, contains 592 809 quasars. This represents roughly a 34% increase with respect to the number of objects recorded in the LQAC-4. Among them, 398 697 objects were found in common with the Gaia DR2, within a 1″ search radius. That corresponds to 67.26% of the whole population of the compilation. Conclusion. The LQAC-5 delivers a nearly complete catalogue of spectroscopically confirmed quasars (including a small proportion of 14 126 compact AGN’s) to the astronomical community, with the aim of giving their best equatorial coordinates with respect to the ICRF2 and with exhaustive additional information. For more than 50% of the sample, these coordinates are extracted from the very recent Gaia DR2.


2019 ◽  
Vol 99 (4) ◽  
pp. 579-583
Author(s):  
X.M. Yang ◽  
C.F. Drury ◽  
W. Xu ◽  
M. Reeb ◽  
T. Oloya

Mid-infrared spectroscopy in the transmission mode was used to predict inorganic nitrogen (N), organic N, and total N in soil leachate. The developed predictions were accurate and robust for total N, NH4+, NO3−, inorganic N (NH4+ + NO3−), and organic N (total N − inorganic N) with high determination coefficients (R2 = 96.7 − 99.0) and residual prediction deviation (RPD = 5.47 − 9.96). The proposed method simultaneously estimates the concentrations of dissolved nitrogen species in soil leachates accurately and with significant savings in time, cost, and chemicals relevant to conventional methods.


2020 ◽  
Vol 498 (4) ◽  
pp. 4721-4744
Author(s):  
F A Olguin ◽  
M G Hoare ◽  
K G Johnston ◽  
F Motte ◽  
H-R V Chen ◽  
...  

ABSTRACT We have studied the dust density, temperature, and velocity distributions of the archetypal massive young stellar object (MYSO) AFGL 2591. Given its high luminosity ($L=2\times 10^5\, \mbox{L$_{\odot}$}$) and distance (d = 3.3 kpc), AFGL 2591 has one of the highest $\sqrt{L}/d$ ratio, giving better resolved dust emission than any other MYSO. As such, this paper provides a template on how to use resolved multiwavelength data and radiative transfer to obtain a well-constrained 2D axisymmetric analytic rotating infall model. We show for the first time that the resolved dust continuum emission from Herschel 70- μm observations is extended along the outflow direction, whose origin is explained in part from warm dust in the outflow cavity walls. However, the model can only explain the kinematic features from CH3CN observations with unrealistically low stellar masses (<15 M⊙), indicating that additional physical processes may be playing a role in slowing down the envelope rotation. As part of our three-step continuum and line fitting, we have identified model parameters that can be further constrained by specific observations. High-resolution mm visibilities were fitted to obtain the disc mass (6 M⊙) and radius (2200 au). A combination of SED and near-infrared observations were used to estimate the luminosity and envelope mass together with the outflow cavity inclination and opening angles.


2017 ◽  
Vol 154 (5) ◽  
pp. 186 ◽  
Author(s):  
Michaela Kraus ◽  
Tiina Liimets ◽  
Cristina E. Cappa ◽  
Lydia S. Cidale ◽  
Dieter H. Nickeler ◽  
...  

2007 ◽  
Vol 3 (S245) ◽  
pp. 451-454
Author(s):  
Georgios E. Magdis ◽  
Dimitra Rigopoulou

AbstractUsing a combination of deep MID-IR observations obtained by IRAC, MIPS and IRS on board Spitzer we investigate the MID-IR properties of Lyman Break Galaxies (LBGs) at z~3, establish a better understanding of their nature and attempt a complete characterisation of the population. With deep mid-infrared and optical observations of ~1000 LBGs covered by IRAC/MIPS and from the ground respectively, we extend the spectral energy distributions (SEDs) of the LBGs to mid-infrared. Spitzer data reveal for the first time that the mid-infrared properties of the population are inhomogeneous ranging from those with marginal IRAC detections to those with bright rest-frame near-infrared colors and those detected at 24μm MIPS band revealing the newly discovered population of the Infrared Luminous Lyman Break Galaxies (ILLBGs). To investigate this diversity, we examine the photometric properties of the population and we use stellar population synthesis models to probe the stellar content of these galaxies. We find that a fraction of LBGs have very red colors and large estimated stellar masses M∗>5×1010M⊙. We discuss the link between these LBGs and submm-luminous galaxies and we report the detection of rest frame 6.2 and 7.7 μm emission features arising from Polycyclic Aromatic Hydrocarbons (PAH) in the Spitzer/IRS spectrum of an infrared-luminous Lyman break galaxy at z=3.01.


2018 ◽  
Vol 612 ◽  
pp. L11 ◽  
Author(s):  
M. Saberi ◽  
W. H. T. Vlemmings ◽  
E. De Beck ◽  
R. Montez ◽  
S. Ramstedt

We present the detection of neutral atomic carbon CI(3P1–3P0) line emission towards omi Cet. This is the first time that CI is detected in the envelope around an oxygen-rich M-type asymptotic giant branch (AGB) star. We also confirm the previously tentative CI detection around V Hya, a carbon-rich AGB star. As one of the main photodissociation products of parent species in the circumstellar envelope (CSE) around evolved stars, CI can be used to trace sources of ultraviolet (UV) radiation in CSEs. The observed flux density towards omi Cet can be reproduced by a shell with a peak atomic fractional abundance of 2.4 × 10−5 predicted based on a simple chemical model where CO is dissociated by the interstellar radiation field. However, the CI emission is shifted by ~4 km s−1 from the stellar velocity. Based on this velocity shift, we suggest that the detected CI emission towards omi Cet potentially arises from a compact region near its hot binary companion. The velocity shift could, therefore, be the result of the orbital velocity of the binary companion around omi Cet. In this case, the CI column density is estimated to be 1.1 × 1019 cm−2. This would imply that strong UV radiation from the companion and/or accretion of matter between two stars is most likely the origin of the CI enhancement. However, this hypothesis can be confirmed by high-angular resolution observations.


Blood ◽  
2014 ◽  
Vol 124 (21) ◽  
pp. 4856-4856
Author(s):  
Peter A. Lane ◽  
Rodney S Theodore ◽  
Maa-Ohui Quarmyne ◽  
James R. Eckman ◽  
Mei Zhou ◽  
...  

Abstract Background: Health services and outcomes research in sickle cell disease (SCD) has been limited by inadequate population-based surveillance and reliance on ICD-9 codes to identify individuals with SCD. The accuracy of ICD-9 coding in administrative claims datasets and the extent of miscoding is unknown. GA was one of 7 states funded to participate in the Registry and Surveillance for Hemoglobinopathies (RuSH) Project. The RuSH case definition for confirmed cases required laboratory documentation of SCD by hemoglobin electrophoresis (HEP)/HPLC. The RuSH case definition for probable cases required identification from administrative datasets of ≥ 2 encounters with an SCD ICD-9 code plus ≥ 1 encounter with ICD-9 or CPT codes from a predetermined list of SCD-associated treatments, procedures, and complications (SCD-TPC): eg hydroxyurea, RBC transfusion, cholecystectomy, stroke. We report results of an ancillary study designed to evaluate the accuracy of using administrative claims data for SCD surveillance by reviewing the medical records (MR) of a large group of children and adolescents identified by SCD ICD-9 codes. Specific objectives were to determine the effect on accuracy of 1) the n of encounters with SCD ICD-9 code for each individual, 2) the addition of SCD-TPC to the case definition, and 3) the length of the surveillance period. We also sought characterize clinical circumstances in which SCD ICD-9 codes were used inaccurately for individuals without SCD. Methods: GA Medicaid (MC) and State Health Benefits Plan (SHBP) databases were used to identify individuals with ≥1 encounter with SCD ICD-9 codes (282.60-282.69; 282.41-282.42) during 2004-2008. The total n of encounters with SCD ICD-9 codes and encounters with SCD-TPC were determined for both a 5-yr (2004-2008) and 1-yr (2008) period. The MR of the subset of children and adolescents seen at Children's Healthcare of Atlanta (CHOA) or Grady were reviewed. Diagnosis of SCD was confirmed by MR review of clinical and laboratory data, including results of newborn screening (NBS), CBC, reticulocytes (retic), and HEP/HPLC. Criteria used to exclude the diagnosis of SCD included 1) absence of any documentation of SCD in provider notes and 2) NBS, HEP/HPLC, and/or CBC/retic results inconsistent with SCD. Cases with MR inadequate to confirm or exclude SCD were categorized as indeterminate. Results: During the 5-yr period 2004-2008, 1,998 children and adolescents with ≥ 1 encounter with SCD ICD-9 code in MC or SHBP datasets were seen at CHOA/Grady, 1,474 (72.8%) of whom had ≥ 1 SCD ICD-9 code during 2008. The Table shows the relationship between the length of the surveillance period and n of encounters with SCD ICD-9 codes in MC/SHBP data sets and SCD status determined by MR review. Abstract 4856. TableSurveillance period (yr)SCD ICD-9 codes (n)PatientsSCDNot SCDIndeterminate5≥ 11,9981,763 (88.2%)196 (9.8%)39 (2.0%)5≥ 21,8511,735 (93.7%)96 (5.2%)20 (1.1%)5≥ 31,7461,693 (97.0%)46 (2.6%)7 (0.4%)1≥ 11,4541,386 (95.3%)57 (3.9%)11 (0.8%)1≥ 21,3731,333 (97.1%)33 (2.4%)7 (0.5%)1≥ 31,2481,231 (98.6%)14 (1.1%)3 (0.2%) For the 5-yr surveillance period, the accuracy of ≥ 2 SCD ICD-coded encounters (93.7%) increased to (97.0%) with addition ≥ 1 encounter with SCD-TPC (RuSH probable case definition), but the number of missed cases increased from 28 (1.6%) to 251 (14.2%). For the 1-yr surveillance period, the same comparison increased the accuracy from 97.1% to 98.4%, but the number of missed cases of SCD increased from 53 (3.8%) to 329 (23.7%). Of 196 patients inaccurately identified as SCD by ICD-9 coding, 65 (33.2%) were hemoglobinopathy carriers; 11 (5.6%) had non-sickle hemoglobinopathies (e.g. HbCC), 9 (4.6%) thalassemias, 18 (9.2%) other non-malignant hematologic disorders, and 19 (9.7%) malignant disorders. Conclusions: Use of administrative claims data to identify children and adolescents with SCD based on ICD-9 coding has important limitations. Accuracy of identification correlated directly with the n of encounters with SCD ICD-9 codes and indirectly with the length of the surveillance period. The addition of ≥ 1 encounter with SCD-TPC to a case definition of ≥ 2 encounters with SCD ICD-9 codes minimally improved specificity but resulted in a large number of missed cases. False positive identification of SCD by ICD-9 coding occurred most commonly in hemoglobinopathy carriers and those with non-sickle hematologic and malignant disorders. Disclosures No relevant conflicts of interest to declare.


2021 ◽  
Vol 162 (4) ◽  
pp. 150
Author(s):  
Michaela Kraus ◽  
Tiina Liimets ◽  
Alexei Moiseev ◽  
Julieta P. Sánchez Arias ◽  
Dieter H. Nickeler ◽  
...  

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