SimDAL Data Access service for AMES-cond evolutionary tracks
Short Name:
AMES-cond tck
Date:
14 Mar 2019 08:14:12
Publisher:
SVO CAB
Description:
SimDAL data access service for AMES-cond evolutionary tracks. Dust in equilibrium with gas phase, with dust opacities ignored, (only GNS1993 available) valid for Teff smaller than 1400 K
SimDAL Data Access service for AMES-cond isochrones
Short Name:
AMES-cond iso
Date:
14 Mar 2019 08:14:12
Publisher:
SVO CAB
Description:
SimDAL data access service for AMES-cond isochrones. Dust in equilibrium with gas phase, with dust opacities ignored, (only GNS1993 available) valid for Teff smaller than 1400 K
SimDAL Data Access service for AMES-dusty evolutionary tracks
Short Name:
AMES-dusty tck
Date:
14 Mar 2019 08:14:12
Publisher:
SVO CAB
Description:
SimDAL data access service for AMES-dusty evolutionary tracks. Dust in equilibrium with gas phase, (only GNS1993 available) valid for Near-IR studies with Teff larger than 1700 K
SimDAL Data Access service for AMES-dusty isochrones
Short Name:
AMES-dusty iso
Date:
14 Mar 2019 08:14:12
Publisher:
SVO CAB
Description:
SimDAL data access service for AMES-dusty isochrones. Dust in equilibrium with gas phase, (only GNS1993 available) valid for Near-IR studies with Teff larger than 1700 K
SimDAL Search service for AMES-cond isochrones and evolutionary tracks
Short Name:
AMES-cond iso
Date:
14 Mar 2019 08:14:12
Publisher:
SVO CAB
Description:
SimDAL search service for AMES-cond isochrones and evolutionary tracks. Dust in equilibrium with gas phase, with dust opacities ignored, (only GNS1993 available) valid for Teff smaller than 1400 K
SimDAL Search service for AMES-dusty isochrones and evolutionary tracks
Short Name:
AMES-dusty iso
Date:
14 Mar 2019 08:14:12
Publisher:
SVO CAB
Description:
SimDAL search service for AMES-dusty isochrones and evolutionary tracks. Dust in equilibrium with gas phase, (only GNS1993 available) valid for Near-IR studies with Teff larger than 1700 K
Planetary systems are built by planets and planetesimals formed in
circumstellar disks surrounding young pre-main sequence stars. Once in
the main-sequence collisions of planetesimals produce small dust
particles giving rise to the so-called debris disks. The mutual
interaction among planets, planetesimals and debris disks, and with
their host stars determines the fate of planetary systems.
Currently thousands of main-sequence stars are known to host planets and
debris disks. The Solar System with its peculiarities is just one of
such planetary systems. However, only few tens of stars are known to
host simultaneously both planets and debris disks. Therefore, the
study of those systems is particularly valuable to widen our knowledge
of planetary systems and their evolution.
This page just collects some of the properties of the known, to our knowledge,
solar-type stars hosting both planets and debris disk.
The Filter Profile Service provides standardized information, including transmission curves and calibration, about astronomical filters. The service is designed to be compliant to the VO Photometry Data Model.
Mark-I is a solar spectrophotometer located and operated at Observatorio del Teide (Tenerife, Canary Islands, Spain) that provides precise radial velocity observations of the Sun-as-a-star at the Potassium KI 7699A absorption solar line. Observations extend from 1976 to 2012 with only summer campaigns from 1976 to 1983.