Neutron stars and stellar-mass black holes are the remnants of massive star explosions1. Most massive stars reside in close binary systems2, and the interplay between the companion star and the newly formed compact object has been theoretically explored3, but signatures for binarity or evidence for the formation of a compact object during a supernova explosion are still lacking. Here we report a stripped-envelope supernova, SN 2022jli, which shows 12.4-day periodic undulations during the declining light curve. Narrow Hα emission is detected in late-time spectra with concordant periodic velocity shifts, probably arising from hydrogen gas stripped from a companion and accreted onto the compact remnant. A new Fermi-LAT γ-ray source is temporally and positionally consistent with SN 2022jli. The observed properties of SN 2022jli, including periodic undulations in the optical light curve, coherent Hα emission shifting and evidence for association with a γ-ray source, poin
The instruments aboard Aditya-L1 are precisely calibrated to scrutinise the solar atmosphere, particularly the chromosphere and corona. | Latest News India
Aditya L1 Mission completed its journey to the sun and entered into the halo orbit on January 6. After this, the satellite will continue to revolve around the Sun collecting significant information related to phenomena related to the Sun s surface
Sharing the images on social media platform X, formerly Twitter, ISRO wrote that the images " provide pioneering insights into the intricate details of the Sun's photosphere and chromosphere."