15998( 4) - 26-May-2020 12:43:47 - [ 1] HUBBLE SPACE TELESCOPE OBSERVING PROGRAM 15998 Version: 4 Check-in Time: 26-May-2020 12:43:47 STScI Edit Number: 0 Title Probing Super-Eddington Outflows via Accreting Galactic BeXRBs ------------------------------------------------------------------------------------ Type Cycle GO 27 ------------------------------------------------------------------------------------ Investigators Contact? PI: Dr. Mark Reynolds University of Michigan Y CoI: Mr. Jakob van den Eijnden Universiteit van Amsterdam N CoI: Dr. Nathalie Degenaar Universiteit van Amsterdam N CoI: Dr. Jon Matthew Miller University of Michigan N CoI: Dr. Dominic Walton University of Cambridge N ------------------------------------------------------------------------------------ Abstract Observations of the population of ultra luminous X-ray sources has revealed that at least a subset of this group contains a neutron star primary. Thus, dramatically demonstrating the viability of super-Eddington accretion for this source class. However, the physics of these super-Eddington accretion flows are poorly understood with the sources typically lying at Mpc distances. The population of Galactic Be/X-ray binaries (BeXRBs) are known to have giant outbursts that enter the super-Eddington regime and promise the opportunity to learn much about this mode of accretion. Herein, we propose to obtain simultaneous high resolution X-ray, UV and radio spectroscopy of the next bright Galactic BeXRB to enter a giant outburst when the neutron star will be accreting in the super-Eddington regime. ------------------------------------------------------------------------------------ Observations Description ------------------------ Studies of giant outbursts of other BeXRBs are highly warranted to determine that winds and jets indeed occur simultaneously in the super-Eddington regime. We note that ULXs are too distant to detect a compact radio jet, so determining the co-existence of winds and jets at highly super-Eddington accretion rates can ONLY be achieved with Galactic BeXRBs, as we aim to target with this proposal. To be able to confirm the presence of both winds and jets in the super-Eddington regime, we therefore proposed for and were granted (quasi-simultaneous) Chandra/HETGS, HST/STIS and JVLA observations of the next giant outburst of a BeXRB. In a BeXRB accreting a super Eddington luminosities, we expect the UV emission to evolve when the accretion envelope develops and shields the outer disk from the inner X-ray emitting region, e.g., Shakura & Sunyaev (1973). In this regime we might expect the UV emission to be dominated by the re-reprocessing component detected in soft X-rays. The high S/N and spectral resolution of STIS will be key here as the kinematics of the accretion inflow and wind will be encoded in the spectral lines. Obtaining observational evidence for wind outflows in ULXs is highly challenging due to the high absorption and distance to these systems. However, low resolution HST/ACS prism spectroscopy has had some limited success and demonstrated the presence of a complex highly ionized outflow at these accretion rates (e.g. M81 X-1, Bregman et al., 2012). 15998( 4) - 26-May-2020 12:43:47 - [ 2] We are requesting observations with STIS with the MAMA detector and the E140M grating, which will provide wavelength coverage from 1150 - 1800 Ang . The high dispersion provided by this grating will ensure the safety of the MAMA detector as these sources can be very bright (> 0.06 Jy; lambda_c ~ 2200Ang). In the event of a fainter UV counterpart, a lower resolution grating will be utilized. Accurate flux estimates will be provided by Swift/UVOT observations in support of this program. ------------------------------------------------------------------------------------ 15998( 4) - 26-May-2020 12:43:47 - [ 3] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 3 GRO-J1008-57 STAR, ACCRETION DISK, RA=10H09M46.9645S, J2000 V = 15 +/- 0.5 ~0.01 mJy at 2000 Ang 1 BE, X-RAY TRANSIENT DEC=-58D17'35.60" Reference Frame: ICRS Extended: NO Comments: This object was generated by the target selector and retrieved from the SIMBAD database. Observation awarded through CXO program. Observation to occur quasi-simultaneously with CXO (+\- 1 day). The source is currently undergoing a large type-II outburst. The program has been triggered. Further trigger details should come via CXO. Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2015.5 -6.144413189254082E-4 0.0035459999999999997 0.0 ------------------------------------------------------------------------------------------------------------------------------------ 15998( 4) - 26-May-2020 12:43:47 - [ 4] TARGET LIST Generic Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Selection Criteria | Flux data No | Name | Description | | ------------------------------------------------------------------------------------------------------------------------------------ 1 BEXRB-TOO STAR, ACCRETION DISK, OTHER: NEXT TYPE-II BEXRB OUTBURST V = 10 ~60 mJy at 2200 Ang BE, X-RAY TRANSIENT Comments: We request a single trigger in cycle 27 to occur quasi-simultaneously with a CXO and VLA observation. We have an approved program with Swift to monitor a bright outburst from a Be/X-ray binary, via 40 monitoring observations. The spectra provided by Swift will be used in combination with data from Swift/BAT and MAXI to trigger the proposed Chandra/HST/JVLA observation. We will trigger this program based on an observation of a known BeXRB at a luminosity in excess of 50% Eddington, e.g., see the BeXRB catalogue1 (Raguzova et al. 2005) or the ESO BeXRB monitor2 . Based on the typical duration of a large outburst (30 - 90 days), we estimate a required turn around time of 21 days, i.e., medium in CXO parlance. The program trigger will come via the CXO office. ------------------------------------------------------------------------------------------------------------------------------------ 15998( 4) - 26-May-2020 12:43:47 - [ 5] Visit: 01 (Orbit 1) Visit Requirements: ON HOLD ; TOO RESPONSE TIME 21.0D On Hold Comments: This cycle 27 HST/STIS observation is on hold pending trigger of our CXO TAC awarded joint CXO/HST/JVLA observation We have an approved program with Swift to monitor a bright out-burst from a Be/X-ray binary, via 40 monitoring observations. The spectra provided by Swift will be used in combination with data from Swift/BAT and MAXI to trigger the proposed Chandra/HST/JVLA observation. We will trigger this program based on an observation of a known BeXRB at a luminosity in excess of 50% Eddington, e.g., see the BeXRB catalogue1 (Raguzova et al. 2005) or the ESO BeXRB monitor2. Based on the typical duration of a large outburst (30 - 90 days), we estimate a required turn around time of ~21 days Additional Comments: The acq exptime is a fiducial configuration given the unknown nature of the target at the current time. Given the system will contain a Be-star, we expect it to be bright (V~10). Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 BEXRB-TOO STIS/CCD ACQ F25ND3 MIRROR 1 1 S (1 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 BEXRB-TOO STIS/FUV ACCUM 0.1X0.03 E140M 1425 1 1000 S -MAMA (1000 S) ------------------------------------------------------------------------------------------------------------------------------------ 3 BEXRB-TOO STIS/FUV ACCUM 0.1X0.03 E140M 1425 1 1040 S -MAMA (1040 S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ BEXRB-TOO 1 STIS/CCD ACQ F25ND3 MIRROR none none none none 1 N/A BEXRB-TOO 2 STIS/FUV ACCUM 0.1X0.03 E140M 1425 none none none none 1 N/A -MAMA BEXRB-TOO 3 STIS/FUV ACCUM 0.1X0.03 E140M 1425 none none none none 1 N/A -MAMA 15998( 4) - 26-May-2020 12:43:47 - [ 6] Visit: 02 (ToO) Visit Requirements: On Hold Comments: Additional Comments: The acq exptime is a fiducial configuration given the previously unknown nature of the target. Given the actual target -- GRO J1008-57 -- has V ~ 14, this needs to be potentially updated. The grating option has been changed to G140L as the source is extincted and has measured Swift/UVOT fluxes during previous outbursts of ~0.01mJy @2000 Ang. We expect a S/N of ~3 in the continumm in 1ks. Line emission from the accretion flow is expected on top of this. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 GRO-J1008-5 STIS/CCD ACQ F28X50LP MIRROR 1 0.5 S (0.5 71 S) ------------------------------------------------------------------------------------------------------------------------------------ 2 GRO-J1008-5 STIS/FUV ACCUM 52X0.2 G140L 1425 1 811 S (811 71 -MAMA S) Comments: Grating changed to G140L as the source is extincted and has measured Swift/UVOT fluxes during previous type II outbursts of ~0.01mJy @2000 Ang. We expect a S/N of ~3 in the continumm in 1ks. Line emission from the accretion flow is expected on top of this. ------------------------------------------------------------------------------------------------------------------------------------ 3 GRO-J1008-5 STIS/FUV ACCUM 52X0.2 G140L 1425 WAVECAL=NO 1 811 S (811 71 -MAMA S) ------------------------------------------------------------------------------------------------------------------------------------ 4 GRO-J1008-5 STIS/FUV ACCUM 52X0.2 G140L 1425 1 811 S (811 71 -MAMA S) ------------------------------------------------------------------------------------------------------------------------------------ 5 WAVE STIS/FUV ACCUM 52X0.2 G140L 1425 1 DEF (0 S) -MAMA ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ GRO-J1008-571 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A GRO-J1008-571 2 STIS/FUV ACCUM 52X0.2 G140L 1425 none none none none 1 N/A -MAMA GRO-J1008-571 3 STIS/FUV ACCUM 52X0.2 G140L 1425 none none none none 1 N/A -MAMA GRO-J1008-571 4 STIS/FUV ACCUM 52X0.2 G140L 1425 none none none none 1 N/A -MAMA WAVE 5 STIS/FUV ACCUM 52X0.2 G140L 1425 none none none none 1 N/A -MAMA 15998( 4) - 26-May-2020 12:43:47 - [ 7] Summary Form for Proposal 15998 Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Apertures 0.1X0.03, 52X0.2, F25ND3, F28X50LP ------------------------------------------------------------------------------------------------------------------------------------ Configurations STIS/CCD, STIS/FUV-MAMA ------------------------------------------------------------------------------------------------------------------------------------ Opmodes ACCUM, ACQ ------------------------------------------------------------------------------------------------------------------------------------ Optional Parameters WAVECAL=NO ------------------------------------------------------------------------------------------------------------------------------------ Special Requirements ON HOLD , TOO RESPONSE TIME 21.0D ------------------------------------------------------------------------------------------------------------------------------------ Spectral Elements E140M, G140L, MIRROR ------------------------------------------------------------------------------------------------------------------------------------ Target Names BEXRB-TOO, GRO-J1008-571, WAVE ------------------------------------------------------------------------------------------------------------------------------------