![]() The information shown is as on Jun 25, 2022. Ĭurrent status of ENIGMA PROPERTIES PRIVATE LIMITED is - ACTIVE. For any Query You can reach this company by email address or Postal address.ĮNIGMA PROPERTIES PRIVATE LIMITED's Annual General Meeting (AGM) was last held on and as per records from Ministry of Corporate Affairs (MCA), its balance sheet was last filed on Mar 31, 2015.ĭirectors of ENIGMA PROPERTIES PRIVATE LIMITED areĪMITAVA CHATTOPADHYAY, RANGASWAMY HARIRAJAN, ROLI AGGARWAL. Its Email address is and its registered address is where Company is actual registered : ECE HOUSE28, K.G MARG New Delhi, Central Delhi, INDIA 110001. 100000.Īs Per Registration of Company, It involves under in Business Activity Class / Subclass Code 45201, Main Activity of the said Company ENIGMA PROPERTIES PRIVATE LIMITED is :, General construction (including alteration, addition, repair and maintenance) of residential buildings, carried –out on own-account basis or on a fee or contract basis., It Comes Under Division CONSTRUCTION and this come under scetion CONSTRUCTION.ĮNIGMA PROPERTIES PRIVATE LIMITED Corporate Identification Number is U45201DL2006PTC147522 and its registration number is 147522. As regarding the financial status on the time of registration of ENIGMA PROPERTIES PRIVATE LIMITED Company its authorized share capital is Rs. ENIGMA PROPERTIES PRIVATE LIMITED is classified as Non-govt company and is registered at Registrar of Companies located in ROC-DELHI. The shape of the 10um silicate feature at this outstanding region.ENIGMA PROPERTIES PRIVATE LIMITED is a Private Company, who was incorporated 16 Year(s) 5 Month(s) 20 Day(s) ago on dated 1. Ourįindings suggest further studies of the composition of interstellar dust and Is an indispensable tool to investigate sources at the Galactic Center. We haveĭemonstrated that optical long baseline interferometry at infrared wavelengths This indicates physically and chemically distinctĬonditions of the local dust, changing with the distance to IRS3. The silicateĪbsorption most probably takes place in the outer diffuse dust, which is mostly Despite observed deep silicate absorption towards IRS3 we favorĪ carbon rich chemistry of the circumstellar dust shell. The IF data resolve the innermost area ofĭust formation. The coinciding interpretation of multiple datasets confirm dustĮmission at several spatial scales. The luminosity and size estimates show that IRS3 is probably a coolĬarbon star enshrouded by a complex dust distribution. Were added to enable simple SED- and full radiative transfer-models of theĭata. That compact 10um source, still unresolved by a single VLT. VLTI/MIDI instrument was used to measure visibilities at 10mas resolution of Imaging separates a compact source from diffuse, surrounding emission. Properties as spectroscopic and interferometric reference star at 10um. Initiated an interferometric experiment to understand IRS3 and investigate its Knowledge of star and dust formation close to a supermassive black hole. The properties ofĮxtreme individual objects of the central stellar cluster contribute to our Spectroscopy failed to solve the enigma of its nature. Robberto Download PDF Abstract: GCIRS3 is the most prominent MIR source in the central pc of the Galaxy.
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