A dataset provided by the European Space Agency

Name OT2_nbillot_2
Title HYSOVAR II: Spectroscopic monitoring of far-IR-variable protostars.
URL

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DOI https://doi.org/10.5270/esa-cl5as7l
Author billot, n.
Description We have recently obtained PACS/Photometer monitoring observations of 100 protostars in the ORION A molecular ridge as part of the program OT1_nbillot_1. We have built about 20 reliable light curves at 70 micron spanning a period of 2 months. We find that a dozen protostars exhibit measurable variability, with flux amplitude of up to 20%, on weekly to monthly timescales. In some cases, the 160 micron light curve also shows variability with amplitude in excess of 10%. For a couple of sources, the 70 and 160 micron light curves appear to be in phase. The observed timescales are orders of magnitude shorter than the dynamical timescales of far-IR emitting material around protostars, which suggests that the mechanism responsible for the far-IR variability might originate from the inner region of the protostars. We have identified a couple of scenarios that could explain the observed far-IR variability, specifically the accretion luminosity variations originating from the inner disk that could lead to the heating of the entire envelope, and thus cause the far-IR variability. The other scenario involves a variable scale height of the disk inner edge that would cast a shadow on the outer disk and inner wall of the envelop cavity. Several of the far-IR variable protostars have already been observed with the PACS/Spectrometer as part of the HOPS program (KPOT_tmegeath_2). Some of the HOPS targets show rich spectra with multiple water and CO lines diagnostic of the activity of infalling envelopes, disks, envelope-disk accretion, and outflows. We propose a small (14.5 hours) exploratory program with the PACS/Spectrometer to monitor the physical and chemical conditions that prevail in the outer disk and envelope of a couple of far-IR variable protostars over a 2-months period.
Publication
    Instrument PACS_PacsRangeSpec_point
    Temporal Coverage 2012-02-26T04:13:55Z/2012-04-15T18:32:43Z
    Version SPG v14.2.2
    Mission Description Herschel was launched on 14 May 2009! It is the fourth cornerstone mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
    Creator Contact https://support.cosmos.esa.int/h®erschel/
    Date Published 2012-10-15T18:16:35Z
    Last Update 2026-03-02
    Keywords Herschel Space Observatory data, ESA Herschel mission dataset, far-infrared astronomy observations, submillimeter astronomy data, infrared space telescope observations, PACS photometer data, PACS spectrometer data, SPIRE photometer data, SPIRE Fourier transform spectrometer data, HIFI heterodyne spectroscopy data, far-infrared spectroscopy dataset, submillimeter spectral line observations, cold universe observations dataset, star formation infrared data, molecular cloud far-infrared observations, interstellar medium spectroscopy data, protoplanetary disk infrared observations, galaxy evolution far-infrared data, dust emission submillimeter observations, cosmic infrared background measurements, extragalactic infrared survey data, calibrated level 2 data products, FITS files astronomy, spectral cubes far-infrared, flux-calibrated maps, continuum photometry data, spectral energy distribution measurements, ESA Herschel Science Archive data
    Publisher And Registrant European Space Agency
    Credit Guidelines European Space Agency, billot et al., 2012, 'HYSOVAR II: Spectroscopic monitoring of far-IR-variable protostars.', SPG v14.2.2, European Space Agency, https://doi.org/10.5270/esa-cl5as7l