On the possibility of faint molecular lines of PO, PH, MgH+, and CN in the solar spectrum
Solar Physics1988Vol. 115(2), pp. 221–227
Citations Over Time
Related Papers
- → A 62 Day X‐Ray Periodicity and an X‐Ray Flare from the Ultraluminous X‐Ray Source in M82(2006)91 cited
- → Origin of the X‐Ray Quasi‐periodic Oscillations and Identification of a Transient Ultraluminous X‐Ray Source in M82(2007)52 cited
- → The rare X-ray flaring activity of the ultraluminous X-ray source NGC 4559 X7(2021)18 cited