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Browsing Aryabhatta Research Institute of Observational Sciences by Author "Kandpal, C. D."

Browsing Aryabhatta Research Institute of Observational Sciences by Author "Kandpal, C. D."

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  • Joshi, S. C.; Srivastava, J. B.; Padalia, T. D.; Kandpal, C. D. (1988)
    Positions of comet Wilson have been measured from the photographic plates taken at the Cassegrain focus of the 104-cm reflector of Uttar Pradesh State Observatory, Naini Tal.
  • Srivastava, J. B.; Kandpal, C. D. (1986)
    Photoelectric observations of WX Eridani in B and V filters have been discussed. The maximum magnitudes of the system are B= 9. ͫ 70 and V= 9. ͫ 46. the B-V colours of the components are 0. ͫ 16 and 0. ͫ 80 for the ...
  • Srivastava, J. B.; Kandpal, C. D. (1981)
    The eclipsing binary AV Hya has been observed photoelectrically in U, B and V filters on 15 nights. The primary eclipse appeared to be total with a totality of 23 min duration. A modified period of 0.6 834 062 has been ...
  • Srivastava, J. B.; Kandpal, C. D. (1987)
    Photometric observations of primary minimum in U, B, and V filters have been discussed. The amplitude of variation in all three filter is 0.ͫ66. We do not find variations in the period and its revised value is 0.ͩ0047115.
  • Srivastava, J. B.; Kandpal, C. D. (1984)
    The star HD 126200 (= BD+8°2857) has now been listed by Kukarkin et al. (1982) as a suspected eclipsing binary of Algol type with a variation of 0.5 magnitude based on the findings of Sanding (1951). Hirschfeld and Sinnott ...
  • Srivastava, J. B.; Kandpal, C. D. (1987)
    The eclipsing binary AY Cam (= BV 363 = BD + 77° 0328) was discovered by Strohmeier and Knigge (1961). They assigned it a period of 1ͩ. 367485. The photographic light curve is of Algol type with no indication of secondary ...
  • Kandpal, C. D. (1976)
    A slightly improved period of 1. ͩ 884 761 9, has been given for the system AO Mon. Photoelectric elements have been computed in B and V filters. The orbit is found to be eccentric. Absolute elements have been derived by ...
  • Srivastava, J. B.; Kandpal, C. D. (1979)
    The light curve and U, B and V observations of the system XY Cep have been presented. Photoelectric and absolute elements of the system have been determined. It is a semi-detached system.
  • Srivastava, J. B.; Kandpal, C. D. (1981)
    VZ Cas is a Mira-type variable star with a period of 169.28d. The spectral type of the star is M0e-M3e. The magnitude is 9.3m - 13.3m (Kukarkin et al., 1976). The star VZ Cas was observed as comparison for the ...
  • Kandpal, C. D.; Srivastava, J. B. (1980)
    Limiting photometric solutions for the system CD Eri in B and V filters have been obtained. The secondary minimum was found to be absent.
  • Joshi, S. C.; Srivastava, J. B.; Kandpal, C. D.; Padalia, T. D.; Sanwal, B. B.; Chaubey, U. S.; Singh, M. (1987)
    Positions of Comet Halley have been measured from the photographic plates taken at Cassegrain focus the 104-cm telescope of Uttar Pradesh State Observatory.
  • Srivastava, J. B.; Kandpal, C. D. (1984)
    The light curves and U, B, and V observations of the system AE Cas have been presented. An improved period of 0ͩ.7591215 is given on the basis of present observations. Photometric elements of the system have been obtained ...
  • Kandpal, C. D. (1975)
    Photoelectric elements of the system TW Cas have been determined in U,B and V filters. A refined period of 1ᵈ.428 324 77 has been given though no change in period is noticed. Spectroscopic elements given by struve have ...
  • Srivastava, J. B.; Kandpal, C. D. (1990)
    Photoelectric observations of eclipsing binary RS CVn carried out at Uttar Pradesh State Observatory Nainital, have been reported. The light curve shows wave-like distortion. Colours and magnitudes of RS CVn and comparison ...
  • Srivastava, J. B.; Kandpal, C. D. (1993)
    Photometric observations of FW Monocerotis in U, B, and V filter have been discussed. The depths of the primary minimum in UBV colours are 2.ᵐ63, 2.ᵐ17 and 1.ᵐ76, respectively. No variation in the period has been found and ...
  • Srivastava, J. B.; Kandpal, C. D. (1988)
    U, B, and V observations of RZ Eri have been reported. COlours of comparison stars BD-10°994, BD-10°996 and of the variable RZ Eri have been presented. The observations of RZ Eri do not indicate the distortion wave in the ...

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