scholarly journals Analysis and test of the central-blue-spot infall hallmark (Corrigendum)

2021 ◽  
Vol 647 ◽  
pp. C2
Author(s):  
R. Estalella ◽  
G. Anglada ◽  
A. K. Díaz-Rodríguez ◽  
J. M. Mayen-Gijon
Keyword(s):  
PEDIATRICS ◽  
1969 ◽  
Vol 44 (5) ◽  
pp. 768-769
Author(s):  
M. Klein ◽  
D. Whelan ◽  
C. Clow ◽  
C. Scriver

In our laboratory, we have been troubled by difficulties in the interpretation of alcian blue and toluidin blue spot tests for mucopolysacchanide disorders. We have tried to provide the clinician with information that would assist him in diagnosis, but were hampered by the apparent high incidence of "false positive" tests. In response to this problem, we reviewed our expenience with 67 referred patients and with 181 retarded institutionalized patients. A positive correlation between test results and chemical disease was found mainly in patients where the diagnosis of mucopolysaccharidosis was already obvious.


2020 ◽  
Vol 48 (1) ◽  
pp. 465-489 ◽  
Author(s):  
David J. Stevenson

Jupiter is in the class of planets that we call gas giants, not because they consist of gas but because they were primarily made from hydrogen-helium gas, which upon gravitational compression becomes a metallic fluid. Juno, in orbit about Jupiter since 2016, has changed our view: The gravity data are much improved, and the simplest interpretation of the higher order even harmonics implies that the planet may have a diluted central concentration of heavy elements. Jupiter has strong winds extending to perhaps ∼3,000-km depth that are evident in the odd zonal harmonics of the gravity field. Jupiter's distinctive magnetic field displays some limited local structure, most notably the Great Blue Spot (a region of downward flux near the equator), and some evidence for secular variation, possibly arising from the winds. However, Juno is ongoing; it has not answered all questions and has posed new ones. ▪  Juno's mission reveals Jupiter's interior. ▪  A core exists but is diluted by hydrogen. ▪  The mission revealed wind depth and magnetic field.


2015 ◽  
Vol 79 (9) ◽  
pp. 1571-1572
Author(s):  
Thomas Middleton ◽  
Aikaterini Dritsoula ◽  
Mahilravi Thevasagayam
Keyword(s):  

2007 ◽  
Vol 32 (1) ◽  
pp. 21-33
Author(s):  
Jacobus W. Mosse ◽  
Campbell R. Davies

The blue spot rock cod, Cephalopholis cyanostigma, is a small common coral reef serranid that forms a significant proportion of the discarded by-catch in the Great Barrier line fishery. Samples were obtained by spear and line fishing at Orpheus Island (range 114- 294 mm FL, mean = 226 mm, n = 137) and from Pelorus Island (range 120-285 mm FL, mean = 214 mm, n = 125). Sagittal otoliths were used to obtain age-based parameter estimates for the populations at each island. Analysis of marginal increments on monthly samples suggested that a single opaque band was deposited annually during November - December. Recaptures of three fishes (9,18, and 24 years old) in July and November 1997, five years after injection of oxytetracycline, further corroborated our conclusion that band formation was annual. The maximum age in our samples of 31 years suggested that the blue spotted rock cod was one of the longest lived serranids documented to date. The von Bertalanffy growth function provided the best description of the pattern of growth for populations at both islands with high coefficients of determination (R2 = 0.86 and 0.82 for Orpheus and Pelorus islands, respectively). Female population of both sites grew relatively slow, not reaching asymptotic size until 7-10 yrs. Statistical comparisons on male and female growth patterns were not significant, however. There were significant differences in growth parameters between islands with C. cyanostigma on average growing larger at Orpheus Island (L?= 258 mm and K= 0.22) compared with Pelorus Island (L?=244 mm and K = 0.25). These age-based population parameter estimates indicated that C. cyanostigma was considerably longer lived than expected for a small coral reef serranid and further demonstrated the utility of age-based methods in studies of the demography of tropical reef fish. The implication for conservation and fisheries management of small tropical serranids is that species with similar population parameters are likely to sustain much lower levels of fishing mortality than previously thought.


2020 ◽  
pp. 509-514

Normal ethnic skin colouration is due to melanin in the skin. However, in this short chapter abnormal blue, grey, or black changes in skin colour, both localized or generalized, are discussed and illustrated by a few clinical images. The Mongolian blue spot that occurs as a physiological change in the skin of the majority of Asian, Black, and Chinese infants is due to melanin. It is uncommon in Caucasian skin types and not always recognized. A good illustration of the relatively common blue naevus is provided and much rarer examples discussed such as naevus of Ota, naevus of Ito, and alkaptonuria. In addition to melanin, other chromophores deposited in the skin may appear blue or black, such as haemoglobin or rarely drug deposits. The popularity of tattoos and associated problems are also mentioned.


2019 ◽  
Vol 626 ◽  
pp. A84 ◽  
Author(s):  
R. Estalella ◽  
G. Anglada ◽  
A. K. Díaz-Rodríguez ◽  
J. M. Mayen-Gijon

Aims. The infall of material onto a protostar, in the case of optically thick line emission, produces an asymmetry in the blue- and red-wing line emissions. For an angularly resolved emission, this translates in a blue central spot in the first-order moment (intensity weighted velocity) map. Methods. An analytical expression for the first-order moment intensity as a function of the projected distance was derived, for the cases of infinite and finite infall radius. The effect of a finite angular resolution, which requires the numerical convolution with the beam, was also studied. Results. This method was applied to existing data of several star-forming regions, namely G31.41+0.31 HMC, B335, and LDN 1287, obtaining good fits to the first-order moment intensity maps, and deriving values of the central masses onto which the infall is taking place (G31.41+0.31 HMC: 70–120 M⊙; B335: 0.1 M⊙; Guitar Core of LDN 1287: 4.8 M⊙). The central-blue-spot infall hallmark appears to be a robust and reliable indicator of infall.


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