Infrared observations of the flaring maser source G358.93-0.03: SOFIA confirms an accretion burst from a massive young stellar object

Autor: Mark Gurwell, Hendrik Linz, J.L. Van der Walt, Claudia Cyganowski, C. Fischer, A. E. Volvach, Gabriele Surcis, Ross A. Burns, Andrej M. Sobolev, V. Wolf, J. Eislöffel, Sylvio Klose, O. Bayandina, Bringfried Stecklum, Crystal L. Brogan, Koichiro Sugiyama, A. Caratti o Garatti, G. C. MacLeod, Gabor Orosz, Yoshinori Yonekura, Kee-Tae Kim, S. Schmidl, Naomi Hirano, Karl M. Menten, M. Olech, Todd R. Hunter, T. K. Sridharan
Přispěvatelé: ITA, USA, GBR, DEU, CAN, TWN, KOR, JPN, IRL, NLD, POL, CHN, ZAF, RUS, University of St Andrews. School of Physics and Astronomy
Jazyk: angličtina
Rok vydání: 2021
Předmět:
GAMMA RAYS
SPECTROMETERS
Young stellar object
DUST
Astrophysics
RADIATIVE TRANSFER
ENVIRONMENTAL CHARACTERISTIC
01 natural sciences
INTERFEROMETRIC IMAGING
RADIATIVE TRANSFER MODEL
law.invention
Luminosity
law
QB Astronomy
Astrophysics::Solar and Stellar Astrophysics
Maser
FIR FILTERS
010303 astronomy & astrophysics
QC
QB
Physics
SPECTROSCOPY
3rd-DAS
ATACAMA LARGE MILLIMETER/SUB-MILLIMETER ARRAYS
FIELD-IMAGING FAR-INFRARED LINE SPECTROMETERS
LUMINANCE
Astrophysics - Solar and Stellar Astrophysics
SPECTRAL ENERGY DISTRIBUTION
Spectral energy distribution
METHANOL
Astrophysics::Earth and Planetary Astrophysics
Flare
ACCRETION
ACCRETION DISKS

INFRARED DEVICES
INDIVIDUAL: G358.93-0.03 [STARS]
Astrophysics::High Energy Astrophysical Phenomena
MASERS
FOS: Physical sciences
Context (language use)
Astrophysics::Cosmology and Extragalactic Astrophysics
Submillimeter Array
indvididual objects (G358.93-0.03) [Stars]
FORMATION [STARS]
0103 physical sciences
INTEGRAL FIELD SPECTROSCOPY
Solar and Stellar Astrophysics (astro-ph.SR)
Astrophysics::Galaxy Astrophysics
PROTOSTARS [STARS]
STRATOSPHERIC OBSERVATORY FOR INFRARED ASTRONOMIES
010308 nuclear & particles physics
Astronomy and Astrophysics
GIANT STARS
Accretion (astrophysics)
QC Physics
13. Climate action
Space and Planetary Science
Zdroj: Astron. Astrophys.
Astronomy and Astrophysics
Popis: Class II methanol masers are signs of massive young stellar objects (MYSOs). Recent findings show that MYSO accretion bursts cause flares of these masers. Thus, maser monitoring can be used to identify such bursts. Burst-induced SED changes provide valuable information on a very intense phase of high-mass star formation. In mid-January 2019, a maser flare of the MYSO G358.93-0.03 was reported. ALMA and SMA imaging resolved the core of the star forming region and proved the association of the masers with the brightest continuum source MM1. However, no significant flux rise of the (sub)mm dust continuum was found. Thus, we performed NIR imaging with GROND and IFU spectroscopy with FIFI-LS aboard SOFIA to detect possible counterparts to the (sub)mm sources, and compare their photometry to archival measurements. The comparison of pre-burst and burst SEDs is of crucial importance to judge whether a luminosity increase due to the burst is present and if it triggered the maser flare. The FIR fluxes of MM1 measured with FIFI-LS exceed those from Herschel significantly, which clearly confirms the presence of an accretion burst. The second epoch data, taken about 16 months later, still show increased fluxes. Our RT modeling yielded major burst parameters and suggests that the MYSO features a circumstellar disk which might be transient. From the multi-epoch SEDs, conclusions on heating and cooling time-scales could be drawn. Circumstances of the burst-induced maser relocation have been explored. The verification of the accretion burst from G358 is another confirmation that Class II methanol maser flares represent an alert for such events. The few events known to date already indicate that there is a broad range in burst strength and duration as well as environmental characteristics. The G358 event is the shortest and least luminous MYSO accretion burst so far.
Comment: 22 pages, 11 figures, accepted by A&A. Abstract abridged for arxiv submission
Databáze: OpenAIRE