Star formation in blue compact dwarf galaxies: Mkn 104 and I Zw 97     

S. Ramya  D. K. Sahu  T. P. Prabhu 《Monthly notices of the Royal Astronomical Society》2009,396(1):97-108

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Unusual optical quiescence of the classical BL Lac object PKS 0735+178 on intranight time-scale     

Arti Goyal    Gopal-Krishna  G. C. Anupama  D. K. Sahu  R. Sagar  S. Britzen  M. Karouzos †  M. F. Aller  H. D. Aller 《Monthly notices of the Royal Astronomical Society》2009,399(3):1622-1632

We present the result of our extensive intranight optical monitoring of the well-known low-energy peaked BL Lac (LBL) object PKS 0735+178. This long-term follow-up consists of R -band monitoring for a minimum duration of ∼4 hours, on 17 nights spanning 11 years (1998–2008). Using the CCD as an N-star photometer, a detection limit of around 1 per cent was attained for the intranight optical variability (INOV). Remarkably, an INOV amplitude of  ≥3 per cent  on hour-like time-scale was not observed on any of the 17 nights, even though the likelihood of a typical LBL showing such INOV levels in a single session of  ≳4  hours duration is known to be high  (∼50 per cent)  . Our observations have thus established a peculiar long-term INOV quiescence of this radio-selected BL Lac object. Moreover, the access to unpublished optical monitoring data of similarly high sensitivity, acquired in another programme, has allowed us to confirm the same anomalous INOV quiescence of this LBL all the way back to 1989, the epoch of its historically largest radio outburst. Here, we present observational evidence revealing the very unusual INOV behaviour of this classical BL Lac object and discuss this briefly in the context of its other known exceptional properties.  相似文献   

Study of star formation in NGC 1084     

S. Ramya  D. K. Sahu  T. P. Prabhu 《Monthly notices of the Royal Astronomical Society》2007,381(2):511-524

We present UBVRI broad-band, Hα narrow-band photometry of the star-forming complexes in the infrared bright galaxy NGC 1084. Results of medium-resolution spectroscopy of some of the brighter complexes are also discussed. Spectroscopic data are used to better estimate the internal reddening within the galaxy which is found to be highly variable and to calculate metallicity which is close to the solar value. A diagnostic diagram identifies the shocked regions within this galaxy. The narrow-band Hα flux and its equivalent width are used to determine the star formation rates of the complexes and the distribution of ages. Star formation rates for a few of the complexes are found to be as high as  0.5 M_⊙ yr⁻¹  . The star-forming complexes lie in the age range 3 to 6.5 Myr. A U − B versus V − I colour–colour mixed population model created using the Starburst99 model colours is used to estimate the ages of the stellar populations present within these regions. Using this technique, it is found that the star formation in NGC 1084 has taken place in a series of short bursts over the last 40 Myr or so. It is proposed that the likely trigger for enhanced star formation is merger with a gas-rich dwarf galaxy.  相似文献   

Factor analysis of sphericity and roundness data of clastic quartz grains: Environmental significance     

B.C. Patro  Basanta K. Sahu 《Sedimentary Geology》1974,11(1):59-78

The first four sample statistics of two-dimensional projection sphericity and those of two-dimensional projection roundness of clastic quartz grains belonging to river, beach and eolian environments and to the three size grades 0.350 mm-0.297 mm, 0.297 mm-0.250 mm and 0.250 mm-0.210 mm were subjected to R-mode factor analysis. The results show that the particles of these size grades are carried largely as a traction carpet in the river and beach environments and are carried largely by saltation in the eolian environment. Sorting and abrasion are the causes of areal variation in the mean sphericity and mean roundness of a population, respectively. Selective sorting causes nonnormality in the sphericity distribution, whereas roundness distribution is originally nonnormal. Selective sorting is most effective in the eolian, less so in the beach and least so in the river environment, and consequently sphericity-nonnormality constitutes a valuable parameter for environmental discrimination. Intensity of rounding is highest in the beach, less in the eolian and least in the river environments. Due to its wide variation from environment to environment the mean roundness constitutes a valuable parameter for differentiating different environments. Sphericity variables contribute more to the discrimination of environments than roundness variables.  相似文献   

An advanced soil moisture accounting procedure for SCS curve number method   总被引：2，自引：0，他引：2  

R. K. Sahu  S. K. Mishra  T. I. Eldho  M. K. Jain 《水文研究》2007,21(21):2872-2881

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Massive compact dwarf stars and C-field     

L. P. Singh  P. K. Sahu 《Journal of Astrophysics and Astronomy》1997,18(1):15-21

The effect of C-field in high density matter has been studied. We find that the negative energy and negative pressure of the C-field helps in formation of massive compact stable neutron stars of mass ∼ 0.5 solar mass which is in the range of 0.01 to 1.0 solar mass of recently observed dwarf stars.  相似文献   

El Niño Modoki connection to extremely-low streamflow of the Paranaíba River in Brazil     

Netrananda Sahu  Swadhin K. Behera  J. V. Ratnam  Roberto Valmir Da Silva  Pradipta Parhi  Weili Duan  Kaoru Takara  R. B. Singh  Toshio Yamagata 《Climate Dynamics》2014,42(5-6):1509-1516

Extremely-low discharge events of the Paranaíba River basin during the austral summer season (December–February, DJF), are found to be associated with the Pacific sea surface temperature anomalies resembling the recently identified El Niño Modoki phenomenon. Extreme discharge events are identified based on their persistent flow for 7 days and more after taking retention time into consideration. Ninety percent of the extremely low discharge events during peak streamflow seasons of DJF, are found to occur during the El Niño Modoki years. A diagnostics study of atmospheric anomalies has shown a clear connection between the modified Walker circulation, associated with the El Niño Modoki, and the precipitation anomalies over the Paranaíba River basin. The climate variations have direct relationship with the rainfall. Streamflow variations are considered as the surrogates to rainfalls. Thus, El Niño Modoki phase is important component to understand and predict the streamflow variations in the Paranaíba River basin.  相似文献   

Spatio-temporal variation of biomass burning sources over South and Southeast Asia   总被引：1，自引：0，他引：1  

L. K. Sahu  Varun Sheel 《Journal of Atmospheric Chemistry》2014,71(1):1-19

In this study, we have investigated the seasonality and long-term trends of major biomass burning (BB) sources over South and Southeast Asia (S-SE Asia). The activities of BB and related emissions show bi-modal seasonality in S-SE Asia. From January to May period, the BB dominates in the northern hemisphere parts of S-SE Asia. From July to September, the activities shift to the southern hemisphere where the emissions from Indonesian and Malaysian islands make largest contributions. Overall, the activities of BB are lowest during October–December period in S-SE Asia. The seasonality of BB intensity and rain are just opposite in the phase over India. The climatological (1997–2008) emissions of carbon monoxide (CO), oxides of nitrogen (NOx) and non-methane hydrocarbons (NMHCs) show strong spatio-temporal variation. The trends show large inter-annual variations with highest and lowest values during years 1997 and 2000, respectively. In the southern hemisphere parts of S-SE Asia mainly in Indonesia, the intensity of biomass fires has been modulated by the large scale climatic phenomena like El Niño and Southern Oscillation (ENSO). The annual emissions of trace gases in southern hemisphere region during the El Niño years exceed to those for the normal years. The estimates for northern hemisphere region during the La Niña years were significantly higher than those for the normal years. The Model for Ozone And Related Chemical Tracers (MOZART) simulations of columnar CO and NOx tend to capture the prominent features of BB emissions in S-SE Asia. The impacts of extensive fires in Indonesia during El Niño year of 2006 compared to a normal year of 2005 were clearly seen in the MOZART-4 simulations of both CO and NOx.  相似文献   

Bianchi Type-1 vacuum models in modified theory of general relativity     

R.C. Sahu  U.K. Panigrahi 《Astrophysics and Space Science》2003,288(4):499-508

In this paper, the problem of spatially homogeneous and an isotropic Bianchi type-1 space time with perfect fluid distribution is considered in Barber's second theory of gravitation. To obtain determinate solutions, we have assumed the equation of statep= γρ, 0 ≤ γ ≤ 1. It is observed that the general fluid distribution degenerates isotropic vacuum model whenγ = 1 and Λ < 0. Further it is observed that the vacuum model obtained in case of γ = 0, ρ = 0 andΛ = 0, reduces to well known Kasner model in Einstein's theory. Some physical and geometrical aspects of the models together with singularities in the models are also discussed This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Photometric and spectroscopic evolution of the Type IIP supernova SN 2004et     

D. K. Sahu  G. C. Anupama  S. Srividya  S. Muneer 《Monthly notices of the Royal Astronomical Society》2006,372(3):1315-1324

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