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Iue observations of mg2 emission form miras
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Brugel, Edward W. |
| Copyright Year | 1987 |
| Description | A total of 61 well exposed low dispersion LWP observations were obtained from the brightest normal M-type Mira variables around their pulsation cycles. By observing Mg II throughout the cycle, the intent is to determine the shock luminosity and duration, and the density in the upper atmospheres of Miras. The data also provide a mechanism for probing the radiative cooling in postshock regions of the atmosphere as a function of time. A summary of data acquired for IUE programs SRHLW and MGIEB is presented. |
| File Size | 309924 |
| Page Count | 6 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19870013139 |
| Archival Resource Key | ark:/13960/t2q57gw6k |
| Language | English |
| Publisher Date | 1987-05-10 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Stellar Atmospheres Shock Waves Cooling Emission Spectra Mira Variables Iue Radiative Transfer Magnesium Balmer Series Stellar Luminosity Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |
