Abstract
We use Gaia DR2 data to survey the classic Monoceros OB1 region and look for the existence of a dispersed young population, co-moving with the cloud complex. An analysis of the distribution of proper motions reveals a 20-30 Myr association of young stars, about 300-400 pc away from the far side of the Mon OB1 complex, along the same general line-of-sight. We characterize the new association, Monoceros OB4, and estimate it contains between 1400 and 2500 stars, assuming a standard IMF, putting it on par in size with NGC\,2264. We find from the internal proper motions that Mon OB4 is unbound and expanding. Our results seem to unveil a larger and more complex Monoceros star formation region, suggesting an elongated arrangement that seems to be at least 300 x 60 pc.
| Original language | English |
|---|---|
| Pages (from-to) | L17-L21 |
| Number of pages | 5 |
| Journal | Monthly Notices of the Royal Astronomical Society: Letters |
| Volume | 504 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 31 Mar 2021 |
Keywords
- ISM: individual objects: Monoceros OB1 cloud complex
- Stars: pre-main sequence
- Galaxy: open clusters and association: general
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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Dive into the research topics of 'Monoceros OB4: a new association in Gaia DR2'. Together they form a unique fingerprint.Projects
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The Planet-Disc Connection: Accretion, Disc Structure and Plant Formation
Matsumura, S. (Investigator) & Sicilia Aguilar, A. (Investigator)
Science and Technology Facilities Council
1/04/19 → 30/06/22
Project: Research
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