The multiple young stellar objects of HBC 515: An X-ray and millimeter-wave imaging study in (pre-main sequence) diversity

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Table 3

SMA fit parameters with upper limits determined from the sensitivity of the observation.

	HBC 515Aa	HBC 515Ab	HBC 515 B	HBC 515 C	HBC 515D¹

Continuum centroid RA	–	–	05:54:03.27	05:54:01.90	–
Continuum centroid Dec	–	–	+01:40:26.49	+01:40:27.38	–
1.3 mm continuum flux [mJy]	<2.9	<2.9	29.9	6.5	<7.7
¹²CO flux [mJy km s^-1]	<1.2	<1.2	<1.2	<1.2	<3.2
¹³CO flux [mJy km s^-1]	<1.2	<1.2	<1.2	<1.2	<3.2
Dust mass [M_E]	<13.4	<13.4	139.5	30.4	<36.0
Total disk mass [M_J]	<4.2	<4.2	44.3	9.6	<11.4

Notes.

⁽¹⁾

Upper limits were estimated by scaling the noise by a factor of 2.7 due to the location of HBC 515D (see Sect. 3.2).

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