paper

HD 44892: The youngest (or oldest?) gas-harbouring debris disc around an intermediate mass star

arXiv:2508.19860 · doi:10.1093/mnras/staf2150

Abstract

We present the first detections of gas around a 2.1 Myr old debris disc-bearing intermediate-mass star, HD 44892. Gas is detected both in CO (2-1) emission through ALMA Band 6 observations and in absorption in Ca II K and H, seen with high-resolution UVES spectroscopy. CO and CO (2-1) are not detected. The star exhibits a 12 m fractional excess of , placing it in the transition stage between protoplanetary and debris discs. Our detection of 1.3 mm emission yields the dust mass of 0.0190.009 assuming 115 K temperature. The CO non-detection places an upper limit on CO gas mass of 10 . The CO detection yields a CO gas mass of (7.862.05)10 or (1.620.17)10 assuming a gas temperature of 20 K or 50 K, respectively. These should be considered as lower limits since CO emission may be optically thick. With UVES, we find variability in Ca II K and H lines, which can be interpreted by transiting circumstellar gas, ruling out interstellar absorption as their origin. Both the dust mass, which is within an order of magnitude of HD 141569, and the gas mass derived here indicate a late gas dispersal stage of the protoplanetary disc. Through our analysis we deem the alternative age of 800 Myr unlikely.

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