Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...182l..59v&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 182, no. 2, Aug. 1987, p. L59-L62.
Astronomy and Astrophysics
Astrophysics
22
Diffusion, Interstellar Matter, Magellanic Clouds, Potassium Iodides, Sodium Iodides, Supernovae, Earth Motion, High Resolution, Line Of Sight, Milky Way Galaxy, Solar Spectra, Spectral Bands
Scientific paper
The authors report the results of high resolution and high S/N observations of diffuse interstellar bands (DIBs) towards SN 1987A in the LMC. For the first time they clearly detect the LMC component of the 5780, 5797 and 6284 Å DIBs, and possibly that of 5778 and 6269 Å. Moreover, they observe the Galactic components of the 5778, 5780, 5797, 6283, 6376 and 6379 Å bands, along a line of sight with very low reddening [E(B-V) ≅ 0.07]. The LMC components are generally weaker than the Galactic ones, while the opposite is observed for ISNa I and K I. The band strengths are compared with the total color excess towards the supernova.
Beckman John E.
Crivellari Lucio
Molaro Paolo P.
Vladilo Gg.
No associations
LandOfFree
Detections of diffuse interstellar bands toward the SN 1987A in the Large Magellanic Cloud 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 Detections of diffuse interstellar bands toward the SN 1987A in the Large Magellanic Cloud, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detections of diffuse interstellar bands toward the SN 1987A in the Large Magellanic Cloud will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1339579