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1 & SDPS team T/Herbig AeBe HL Tau, HH30, GM Aur, HD141569, AB Aur disk-planet connection
2 NIR/Mid-IR thermal dust (OIR interferometer, AsAst.) Domain sampled in current images at 150 pc Scattered Light in Optical and NIR (opt. thick) mm / submm thermal dust emission (opt. thin) Optically thick CO lines Accretion shock thin lines Accretion disk ~ Kuiper Belt Vertical scale near the star Stellar magnetosphere Accretion columns (broad emission lines: H, etc) Acc. Rate ~10-8 M /yr Wind Passive reprocessing disk Planetesimals? Flaring Approximate H(r) at 500 AU (AU) ~ 1 Approximate radius r (AU) ~ 50 ~ 100 ~ 500 Adapted from A. Dutrey
3 cold dust hot dust dust dust dust ring, gap, central hole, etc. VLA 7mm 1 SMA(>0.1 )/ALMA(>0.01 )
4 HST WFPC2 ~0.1 some TTS; ACS STIS ~0.1 ACS ~0.05 NICMOS m AO (98%)PSF 1997/3-1998/12: LN2 2002/4 wedge width = 0.5 3
5 mask size = 1.8 & 3.0 NICMOS COOLING SYSTEM The NCS System was flight tested on STS-95 (October 1998) in the Shuttle Bay on NASA/GSFC s Hubble Orbital System s Test (HOST) Pallet.
6 AO0.1 Subaru CIAO/IRCS + 36 AO Keck KCam/NIRC/NIRC2+349AO VLT CONICA+185NAOS (NACO) Gemini Hokupa a 85AO+ CHFTUH-AOADONISIRTF/CoCo T AO VLTAO TTSTTSAO
7 Tamura, Gatley, Werner et al. 1991, ApJ, 374, L25 (w/ 62x58 IR arrays) Tamura et al.
8 IRAS : Butterfly JHK composite; HST/NICMOS 11 x11 (1500AUx1500AU), Padgett et al dark lane edge-on disk (Wood et al. 03) Shakura & Sunyaev 73 Ulrich 76 Outer radius R(out)=300AU disk flaring parameter =1.29 rarial density profile =2.37 scale height h(100au)=15au M(disk)=0.07Mo Ishii, Tamura, & Itoh m
9 Ishii et al IRAS separation=25 AU helical jet? JHK composite, HST/NICMOS 11 x11 (1500AUx1500AU), Padgett et al. 1999
10 HL Tau C: Subaru/CIAO (H) B: HST/WFPC2 (F555W, Stapelfeld 95) 1 =140AU NIR w/ao vs. optical/ space point-like source + envelope two cavities inner flipped-c shape nebula northern arm inner part optical, outer part NIR optical jet* misaligned with the inner cavity (*) optical jet within the inner cavity is not well measured due to color gradient Polarization image of HL Tau Lucas, Fukagawa, Tamura et al. 2004
11 HST/NICMOS a(max)>50m M(disk)>0.0015Mo F675W/F119/F204M composite ~1 x1 (140AUx140AU) Cotera et al Red Polar Lobes 10 µjy arcsec -2 GM AUR Unembedded (A v < 0.5) Coronagraph + PSF Subtraction Lower Scattering Surface 0.2 mjy arcsec -2 Faint Blue Ribbon 140 pc, ctts (K7 V), 0.84 Mo, 1.3 Myr NICMOS / 1.1 & 1.6 m + coronagraph J * = 0.33 Jy H * = 0.40 Jy GM Aur 5 =700AU
12 HD A 99 pc, Herbig Be (B9.5 Ve) HST/ACS + coronagraph STIS/NICMOS dust migration V-band image, HST/ACS Clampin et al AB Aur 144pc, Herbig Ae (A0 Ve), 2.4 Mo, 4Myr SubaruCIAOAO 580 AU Fukagawa et al. 2004
13 Intro: planet & BD direct detections sensitivity, angular resolution, dynamic range aged planets: beyond current instrument power hot jupiters: beyond 8-mAO; go to 8m IR interferometers the younger, the better (both luminosity & dynamic range) current searches: SFRs, nearby clusters Current Status direct planet detections Companion searches around nearby stars HST faint companion (FC) searches around nearby 23 stars with WFPC2 (Schroeder et al. 99) NICMOS survey of 45 young (<300Myr) nearby stars (Lowrance 03) Palomar searches for 8pc sample (Oppenheimer et al. 00) Subaru searches around slow movers (Nakajima et al. planned) Companion searches around Doppler planet stars Keck searches around 25 stars (Luhman & Ray-Jay 00) Lick et al. searches around 11 stars (Patience et al. 02) Companion searches around VLM objects HST searches around VLM objects (eg., Reid et al. 01) Gemini searches around VLM objects (Potter et al. 02; Close et al. 03) BD binaries <NOTE:VLM objects=very Low Mass objects> Companion searches around YSOs or clusters Various searches in Pleiades (Martin et al. 00) ADONIS survey of Tuc-Hor association (Chauvin et al. 03) Subaru searches around 100 stars (Hayashi, Tamura et al. ongoing) Various Free-Floating Planet (aka. Sub-Brown Dwarfs) searches in SFRs No planets except several BDs (e.g., Gl229, Gl86, HD130948, TWA-5, HR 7672) discovered so far.
14 Two ultracool companions to the young star HD Mars orbit at 17pc Pair has same proper motion as primary (7 month basis 148 mas/yr Gravitationally bound pair brown dwarf binary Pair separation = / Subaru/IRCS spectroscopy (Goto et al.) Primary < 1 Gyr TWA-5B (CoD ) 55pc YBD(12MYr) M Jupiter HR 7672B (15 Sge) 18pc ~2GYr for Pr. ~65M Jupiter Gl 86B Gl 229B 11pc several GYr ~50?M Jupiter 11pc MYr?? ~50?M Jupiter
15 T Common proper motion Subaru Disk and Planet Search project disk morphology details AO disk spectroscopy SED
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