VizieR Online Data Catalog: Distances to molecular clouds in SFR (Zucker+, 2020) (2024)

Zucker, C. (Autor*in), Speagle, J. S. (Autor*in), Schlafly, E. (Autor*in), Green, G. M. (Autor*in), Finkbeiner, D. P. (Autor*in), Goodman, A. (Autor*in). (2019). VizieR Online Data Catalog: Distances to molecular clouds in SFR (Zucker+, 2020). Software oder Datenbank http://adsabs.harvard.edu/abs/2019yCat..36330051Z

Zucker, C. (Autor*in) ; Speagle, J. S. (Autor*in) ; Schlafly, E. (Autor*in) et al.. / VizieR Online Data Catalog: Distances to molecular clouds in SFR (Zucker+, 2020). [Software oder Datenbank].

@misc{2a1acb3fdc94485aa2df31e3e7331e22,

title = "VizieR Online Data Catalog: Distances to molecular clouds in SFR (Zucker+, 2020)",

abstract = "Distances to ~60 star-forming regions in Reipurth (2008, Star Formation Handbook, vols I and II) have been computed using stellar photometry and Gaia DR2 parallax measurements. Usually, several distance estimates are taken across each cloud. For each sightline, the median distance (d50) is provided, plus the 16th and 84th percentiles on the distance probability distribution function. There is an additional systematic uncertainty, which is unknown but estimated to be ~5% in distance for clouds 1.5kpc, and ~7% in distance for the southern clouds Lupus, Chamaeleon, and Corona Australis. These should be added in quadrature with the statistical uncertainties reported in the table. In addition to the distances, ancillary model parameters used in our fit are also included (e.g. the amount of foreground extinction {"}f{"}). See Section 3.2.1 and Section 3.2.2 in Zucker et al. (2019ApJ...879..125Z) for a complete description of model parameters. (1 data file).",

keywords = "Molecular clouds, Stars: distances",

author = "C. Zucker and Speagle, {J. S.} and E. Schlafly and Green, {G. M.} and Finkbeiner, {D. P.} and A. Goodman and J. Alves",

year = "2019",

month = sep,

day = "1",

language = "English",

volume = "363",

}

Zucker, C, Speagle, JS, Schlafly, E, Green, GM, Finkbeiner, DP, Goodman, A, VizieR Online Data Catalog: Distances to molecular clouds in SFR (Zucker+, 2020), 2019, Software oder Datenbank. <http://adsabs.harvard.edu/abs/2019yCat..36330051Z>

VizieR Online Data Catalog: Distances to molecular clouds in SFR (Zucker+, 2020). Zucker, C. (Autor*in); Speagle, J. S. (Autor*in); Schlafly, E. (Autor*in) et al.. 2019.

Veröffentlichungen: Elektronische/multimediale Veröffentlichung › Software oder Datenbank

TY - ADVS

T1 - VizieR Online Data Catalog: Distances to molecular clouds in SFR (Zucker+, 2020)

AU - Zucker, C.

AU - Speagle, J. S.

AU - Schlafly, E.

AU - Green, G. M.

AU - Finkbeiner, D. P.

AU - Goodman, A.

AU - Alves, J.

PY - 2019/9/1

Y1 - 2019/9/1

N2 - Distances to ~60 star-forming regions in Reipurth (2008, Star Formation Handbook, vols I and II) have been computed using stellar photometry and Gaia DR2 parallax measurements. Usually, several distance estimates are taken across each cloud. For each sightline, the median distance (d50) is provided, plus the 16th and 84th percentiles on the distance probability distribution function. There is an additional systematic uncertainty, which is unknown but estimated to be ~5% in distance for clouds 1.5kpc, and ~7% in distance for the southern clouds Lupus, Chamaeleon, and Corona Australis. These should be added in quadrature with the statistical uncertainties reported in the table. In addition to the distances, ancillary model parameters used in our fit are also included (e.g. the amount of foreground extinction "f"). See Section 3.2.1 and Section 3.2.2 in Zucker et al. (2019ApJ...879..125Z) for a complete description of model parameters. (1 data file).

AB - Distances to ~60 star-forming regions in Reipurth (2008, Star Formation Handbook, vols I and II) have been computed using stellar photometry and Gaia DR2 parallax measurements. Usually, several distance estimates are taken across each cloud. For each sightline, the median distance (d50) is provided, plus the 16th and 84th percentiles on the distance probability distribution function. There is an additional systematic uncertainty, which is unknown but estimated to be ~5% in distance for clouds 1.5kpc, and ~7% in distance for the southern clouds Lupus, Chamaeleon, and Corona Australis. These should be added in quadrature with the statistical uncertainties reported in the table. In addition to the distances, ancillary model parameters used in our fit are also included (e.g. the amount of foreground extinction "f"). See Section 3.2.1 and Section 3.2.2 in Zucker et al. (2019ApJ...879..125Z) for a complete description of model parameters. (1 data file).

KW - Molecular clouds

KW - Stars: distances

M3 - Software or database

VL - 363

ER -

Zucker C (Autor*in), Speagle JS (Autor*in), Schlafly E (Autor*in), Green GM (Autor*in), Finkbeiner DP (Autor*in), Goodman A (Autor*in) et al.. VizieR Online Data Catalog: Distances to molecular clouds in SFR (Zucker+, 2020) 2019.