Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars.

Pecaut, M. J., & Mamajek, E. E. (2013). Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars. The Astrophysical Journal Supplement Series, 0067-0049.

Type

Journal article

Intellectual base

Primary research

Year

2013

DOI

10.1088/0067-0049/208/1/9

Link

https://doi.org/10.1088/0067-0049/208/1/9

Cited by

2 citations across 2 artifacts.

Each citation links to the sentence it supports in the citing article.

Domain-specific

• A-Type Main-Sequence Star
  • Their adopted median effective temperatures run from about 9700 K at A0 V through 7440 K at A9 V, with intermediate values attached to intermediate standards.
• B-type Main-Sequence Star
  • For approximately solar-composition dwarf calibrations, B0 V through B9 V span roughly 31,400 to 10,700 K and about 17.7 to 2.75 solar masses in the Pecaut–Mamajek sequence; luminosity and radius change by still larger factors.

    This sourceTable 5 includes an empirical dwarf color and temperature sequence used as a calibration source.

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Registry ID ref:070084d2f7ab · see in the full table