Spectroscopic and photometric observations of SN 1987A. IV - Days 260-385

Details Spectroscopic and photometric observations of SN 1987A. IV - Days 260-385 Spectroscopic and photometric observations of SN 1987A. IV - Days 260-385

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.234p...5w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 234, Sept. 1, 1988, p. 5P-18P.

Astronomy and Astrophysics

Astronomy

63

Astronomical Photometry, Astronomical Spectroscopy, Supernova 1987A, Bolometers, Light Curve, Magellanic Clouds

Scientific paper

Spectroscopic and photometric [UBV(RI)cJHKLM] observations of SN 1987A in the Large Magellanic Cloud are described and briefly discussed. These cover the interval from days 260-385 after core collapse. During this period the bolometric light curve, determined from optical and infrared photometry, has been declining slightly faster than the rate expected for the radioactive dacay of 56Co. The flux deficit is, however, compensated for by γ-radiation, indicating that the decay of 56Co continues to be the sole significant energy source of the supernova.

Affiliated with

Also associated with

No associations

Rating

Spectroscopic and photometric observations of SN 1987A. IV - Days 260-385 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectroscopic and photometric observations of SN 1987A. IV - Days 260-385, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic and photometric observations of SN 1987A. IV - Days 260-385 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-914944