Multiwavelength Observations of Two Bright Dust Forming CO Novae: V2362 Cyg and V1280 Sco

Details Multiwavelength Observations of Two Bright Dust Forming CO Novae: V2362 Cyg and V1280 Sco Multiwavelength Observations of Two Bright Dust Forming CO Novae: V2362 Cyg and V1280 Sco

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2354s&link_type=abstract

Chandra Proposal ID #09300509

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Chandra Proposal Id #09300509

Scientific paper

We request two 25 ks HRC-S+LETG observations for each of two slow, dust-forming, carbon-oxygen Classical Novae: V2362 Cyg and V1280 Sco. This will be the first time that this class of novae has been observed in X-rays. This is a Target-of-Opportunity proposal and we will use SWIFT to confirm that each nova is sufficiently bright for a grating spectrum before triggering our Chandra observations. Since the XRT instrument on SWIFT has roughly the same spectral resolution and effective area as ACIS-S on Chandra, the improved spectral resolution of the Chandra gratings is the justification for our observations. We will obtain monitoring observations with SWIFT, with Spitzer, Gemini, and other ground based telescopes.

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