Misfits [part 2 V13.1] -

You can find the full research documentation on the IOPscience portal . THE REAL SOLAR NEIGHBORHOOD PROTOSTARS - IOPscience

The primary goal of the MISFITS survey is to identify and characterize —stars still embedded in dense, infalling envelopes of gas and dust—which have often been misidentified in previous studies. Misfits [Part 2 v13.1]

: A central star and disk embedded within a dense envelope. You can find the full research documentation on

The survey addresses common errors in identifying Young Stellar Objects (YSOs) caused by factors like , which can make older Stage II sources appear younger. The survey addresses common errors in identifying Young

: For a source to be confirmed as a protostar in this survey, the emission must be extended but peaked directly on the source to rule out unrelated nearby emission.

) and submillimeter dust continuum emission to confirm the presence of an extended envelope.

: A star and disk where the envelope has mostly dissipated.