Studies on the inheritance pattern of joints, pod and flower pigmentation in cowpea [Vigna unguiculata (L) walp.]

Genetic studies were carried out to elucidate the inheritance pattern of plant, flower and pod-tip pigmentation in cowpea. The parental varieties were selected based on their contrasting plant and flower pigmentation. These varieties were grown in the screen house between May, 2002 and October, 2003, and sufficient number of parental F1, F2, backcross and F3 seeds were obtained. The F1, F2, and backcross along with parent seed were planted in the field during the cropping season covering July-October, 2003. Observations were taken on joint pigmentation, flower colour and pod traits on individual plant basis in each population. The results were analyzed for genetic segregation, to determine the number of genes controlling these traits and interactions between them. The joint pigmentation was controlled by one dominant gene. The coloured margins on the standard and wings of flower were controlled by one dominant gene; the purple standard and wings was also controlled bya single dominant gene and it was allelic to the gene controlling the coloured margins. The purple wing with white standard was controlled by another dominant gene which was  different from the ones controlling pigments on the standard petal. The pigmented (purple) calyx was controlled by two genes and it was pleiotropic (tightly linked) to pod-tip as well as purple backline on standard petal. Of the two genes controlling the calyx colour, one controls joint pigmentation such that in the absence of joint pigmentation is prerequisite for calyx, pod-tip and backline pigmentation

Mayer-Rokitansky-Kuster-Hauser Type I Syndrome - A Case Report

Mayer-Rokitansky-Kuster-Hauser (MRKH) Syndrome is not uncommon as this is a part of the Mullerian agenesis. This isusually diagnosed during adolescent period when signs and symptoms of the ongoing changes in female body type are delayed.We present 17 years old adolescent female who presented with primary amenorrhoea as the normal menstruation did not startat puberty. She was diagnosed as MRKH Type I Syndrome on the basis of radiological investigations

Importance of Conventional Radiography in Diagnosis and Management of Giant Cell Tumour at an unusual location

Giant cell tumour (GCT) or osteoclastoma of the bone is mostly benign but locally aggressive primary tumour of unknownorigin occurring at epiphysis. It is a tumour of long bones and rarely seen in bones of hand and foot. The cases are reported intarsal and carpal bone but involvement of metatarsal bone is very rare. We present a case of twenty years old female patientwith GCT of second metatarsal of left foot. The patient underwent aggressive curettage and filling with bone chips and is onregular follow up

Radiological diagnosis of Cysticercosis of Breast - An unusual presentation

Breast cysticercosis manifestation is usually uncommon and only a few cases have been reported in the literature. Thismanifests in the form of signs and symptoms which normally do not point towards the diagnosis. The radiological modalitiesalways narrow down the gap between the complaints and the diagnosis. We present a case with cysticercus cysts in breastparenchyma as well as in both pectoral muscles which was suspected on ultrasonography (USG) and diagnosed on MagneticResonance Imaging (MRI). The patient responded to the medical treatment conservatively thus avoiding excisional biopsy.Follow up and repeat MRI has confirmed the cure of the complaints as well as the disease

Bianchi Type-II String Cosmological Models in Normal Gauge for Lyra's Manifold with Constant Deceleration Parameter

The present study deals with a spatially homogeneous and anisotropic Bianchi-II cosmological models representing massive strings in normal gauge for Lyra's manifold by applying the variation law for generalized Hubble's parameter that yields a constant value of deceleration parameter. The variation law for Hubble's parameter generates two types of solutions for the average scale factor, one is of power-law type and other is of the exponential form. Using these two forms, Einstein's modified field equations are solved separately that correspond to expanding singular and non-singular models of the universe respectively. The energy-momentum tensor for such string as formulated by Letelier (1983) is used to construct massive string cosmological models for which we assume that the expansion ($\theta$) in the model is proportional to the component $\sigma^{1}_{~1}$ of the shear tensor $\sigma^{j}_{i}$. This condition leads to $A = (BC)^{m}$, where A, B and C are the metric coefficients and m is proportionality constant. Our models are in accelerating phase which is consistent to the recent observations. It has been found that the displacement vector $\beta$ behaves like cosmological term $\Lambda$ in the normal gauge treatment and the solutions are consistent with recent observations of SNe Ia. It has been found that massive strings dominate in the decelerating universe whereas strings dominate in the accelerating universe. Some physical and geometric behaviour of these models are also discussed.Comment: 24 pages, 10 figure