TY - JOUR
T1 - Outbursting Young Stellar Object PGIR 20dci in the Perseus Arm
AU - Hillenbrand, Lynne A.
AU - De, Kishalay
AU - Hankins, Matthew
AU - Kasliwal, Mansi M.
AU - Rebull, Luisa M.
AU - Lau, Ryan M.
AU - Cutri, Roc M.
AU - Ashley, Michael C.B.
AU - Karambelkar, Viraj R.
AU - Moore, Anna M.
AU - Travouillon, T.
AU - Mainzer, A. K.
N1 - Publisher Copyright:
© 2021. The American Astronomical Society. All rights reserved.
PY - 2021/5
Y1 - 2021/5
N2 - We report the discovery of a likely outbursting Class I young stellar object, associated with the star-forming region NGC 281-W (distance ∼2.8 kpc). The source is currently seen only at infrared wavelengths, appearing in both the Palomar Gattini InfraRed (1.2 μm) and the Near-Earth Object Wide-field Infrared Survey Explorer (3.4 and 4.6 μm) photometric time-domain surveys. Recent near-infrared imaging reveals a new, extended scattered light nebula. Recent near-infrared spectroscopy confirms the similarity of PGIR 20dci to FU Ori-type sources, based on strong molecular absorption in CO, H2O, and OH; weak absorption in several atomic lines; and a warm wind/outflow as indicated by a P Cygni profile in the He i λ10830 line. This is a rare case of an FU Ori star with a well-measured long-term photometric rise before a sharper outburst, and the second instance of an FU Ori star with a documented two-step brightening in the mid-infrared.
AB - We report the discovery of a likely outbursting Class I young stellar object, associated with the star-forming region NGC 281-W (distance ∼2.8 kpc). The source is currently seen only at infrared wavelengths, appearing in both the Palomar Gattini InfraRed (1.2 μm) and the Near-Earth Object Wide-field Infrared Survey Explorer (3.4 and 4.6 μm) photometric time-domain surveys. Recent near-infrared imaging reveals a new, extended scattered light nebula. Recent near-infrared spectroscopy confirms the similarity of PGIR 20dci to FU Ori-type sources, based on strong molecular absorption in CO, H2O, and OH; weak absorption in several atomic lines; and a warm wind/outflow as indicated by a P Cygni profile in the He i λ10830 line. This is a rare case of an FU Ori star with a well-measured long-term photometric rise before a sharper outburst, and the second instance of an FU Ori star with a documented two-step brightening in the mid-infrared.
UR - https://www.scopus.com/pages/publications/85106297548
UR - https://www.scopus.com/pages/publications/85106297548#tab=citedBy
U2 - 10.3847/1538-3881/abe406
DO - 10.3847/1538-3881/abe406
M3 - Article
AN - SCOPUS:85106297548
SN - 0004-6256
VL - 161
JO - Astronomical Journal
JF - Astronomical Journal
IS - 5
M1 - 220
ER -