iSHELL K-band Survey of Class I and Flat Spectrum Sources: Magnetic Field Measurements in the Protostellar Phase
Abstract We perform the first magnetic field strength survey of Class I and Flat Spectrum (FS) sources using K -band observations with iSHELL. We obtained new observations of 42 Class I and FS sources and additionally included 10 sources from the archive. We detect photospheric lines in 44 of the sources, in addition to Br γ , H 2 , and CO emission in several objects. We model the photospheric absorption lines of 32 Class I and FS sources and measure their magnetic field strengths, K -band temperatures, gravities, projected rotational velocities, and infrared veiling values. We put the physical properties of Class I and FS sources in context by comparing them to the values derived for a sample of Class II sources. We find that (a) the average magnetic field strength of Class I and FS sources 〈 B 〉 = 2.0 ± 0.15 kG is consistent with the average magnetic field strength of Class II sources 〈 B 〉 = 1.8 ± 0.15 kG, and (b) the average gravity of Class I and FS objects <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mi>g</mml:mi> <mml:mo>=</mml:mo> <mml:mn>3.43</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.07</mml:mn> </mml:math> is lower than the average gravity of Class II sources <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mi>g</mml:mi> <mml:mo>=</mml:mo> <mml:mn>3.75</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.04</mml:mn> </mml:math> , although there is significant overlap between both gravity distributions. Furthermore, using stellar evolutionary models, we deduce that Class I and FS sources have a median age of ∼0.6 Myr, and are, as a group, younger than the Class II stars with a median age of ∼3 Myr. Our results confirm that Class I and FS sources host strong magnetic fields on their photospheres. Thus, it is likely that these sources accrete disk material through a magnetosphere similar to the more evolved T Tauri stars.
Authors
- A. C. A. Boogert (ORCID: https://orcid.org/0000-0001-9344-0096)
- Christian Flores (ORCID: https://orcid.org/0000-0002-8591-472X)
- Bo Reipurth (ORCID: https://orcid.org/0000-0001-8174-1932)
- Michael S. Connelley (ORCID: https://orcid.org/0000-0002-8293-1428)
- G. Doppmann
Institutions
- University of Hawaiʻi at Mānoa (US)
- Planetary Science Institute (US)
- Institute of Astronomy and Astrophysics, Academia Sinica (TW)
- W.M. Keck Observatory (US)
- East Asian Observatory (US)
Publication Details
- Journal
- The Astrophysical Journal
- Published
- 2024-09-01
- DOI
- https://doi.org/10.3847/1538-4357/ad58b1
- Citations
- 8
- Primary Topic
- Astro and Planetary Science
- Type
- article
- Field-Weighted Citation Impact
- 2.65
Funders
- National Science Foundation
- National Aeronautics and Space Administration
- California Institute of Technology
- Universität Wien
- Uppsala Universitet
- Jet Propulsion Laboratory
- University of California, Los Angeles