Getting SMARTS on Novae: Highlights of the Early Evolution of Nova V475 Sct

Details Getting SMARTS on Novae: Highlights of the Early Evolution of Nova V475 Sct Getting SMARTS on Novae: Highlights of the Early Evolution of Nova V475 Sct

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.304..401s&link_type=abstract

Astrophysics and Space Science, Volume 304, Issue 1-4, pp. 401-403

Astronomy and Astrophysics

Astrophysics

1

Novae, Photometry, Spectroscopy, Light Curves, Line Profiles

Scientific paper

There is a disconcerting global trend of retiring telescopes of modest aperture, supplanting them instead with fewer expensive telescopes of quite large aperture. As a consequence, the available time and feasibility of following transient objects in astrophysics is diminishing. We show the utility of having a suite of small to moderate aperture telescopes capable of conducting imaging and spectroscopic observations in a service queue mode. The example we provide is the high-cadence early observations of the classical nova V475 Scuti (2003) carried out with the SMARTS suite of telescopes located at CTIO.

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